The Cambridge Atlas of Herschel Objects

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The Cambridge Atlas of Herschel Objects This superb, all purpose star atlas is the first of its kind devoted to observing the Herschel objects with binoculars and telescopes. It displays over 2,500 of the most visually attractive star clusters, nebulae, and galaxies that were discovered by Sir William, Caroline, and Sir John Herschel, and is a must have for stargazers who want to explore these fascinating objects. Covering the entire sky from the North to the South Celestial Pole, and showing all 88 constellations, it is also a general sky atlas showing variable, double and multiple stars, and the Milky Way. Written by experienced observer James Mullaney and illustrated by renowned celestial cartographer Wil Tirion, this is a magnificent ‘celestial roadmap’ to some of the finest deep sky showpieces. Spiral bound and printed in red light friendly colors for use at a telescope, with color coded symbols for easy recognition and identification, this is an all purpose observing reference for all amateur observers. james mullaney, a Fellow of the Royal Astronomical Society of London, is an astronomy writer, lecturer, and consultant. He has published more than 500 articles and seven books on observing the wonders of the heavens. wil tirion is a full time uranographer. He is famous for the numerous star charts he has created for astronomy books, atlases, and magazines. The minor planet, 4648 Tirion (1931 UE), is named after him.

THE CAMBRIDGE ATLAS OF

HERSCHEL OBJECTS JAMES MULLANEY, FRAS WIL TIRION

cambridge university press Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore, Sa˜o Paulo, Delhi, Dubai, Tokyo, Mexico City Cambridge University Press The Edinburgh Building, Cambridge CB2 8RU, UK Published in the United States of America by Cambridge University Press, New York www.cambridge.org Information on this title: www.cambridge.org/9780521138178 # J. Mullaney and W. Tirion 2011 This publication is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 2011 Printed in the United Kingdom at the University Press, Cambridge A catalogue record for this publication is available from the British Library Library of Congress Cataloging in Publication Data Mullaney, James, 1940– The Cambridge atlas of Herschel objects / James Mullaney, Wil Tirion. p. cm. ISBN 978 0 521 13817 8 (Pbk.) 1. Stars–Atlases. 2. Stars–Clusters–Atlases. 3. Nebulae–Atlases. 4. Galaxies–Atlases. I. Tirion, Wil. II. Title. QB65.M85 2010 523.8–dc22 2010030380 ISBN 978 0 521 13817 8 Paperback Cambridge University Press has no responsibility for the persistence or accuracy of URLs for external or third party internet websites referred to in this publication, and does not guarantee that any content on such websites is, or will remain, accurate or appropriate.

CONTENTS

Introduction

page 1

Who were the Herschels?

1

The Herschels’ telescopes

2

The Herschel designations

4

Map parameters and selection criteria

6

Instrumental factors

7

Observing hints

9

Herschel showpieces

12

Some recommended references

34

About the authors

36

Acknowledgements

36

Star charts

37

Appendix A: Constellation table

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Appendix B: The Cambridge Atlas of Herschel Objects target list

106

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INTRODUCTION

We are very pleased to present what is the first major star atlas devoted to the observation of the “Herschel objects” – some 5,000 star clusters, nebulae, and galaxies collectively discovered by Sir William Herschel, his sister Caroline, and son Sir John. With the widespread growing popularity of viewing these wonders of the heavens by amateur astronomers today, the need for such a work clearly exists. The one classic atlas that identified some of those objects found by William Herschel, using his designations (329 of them), was Norton’s Star Atlas in all of its first 17 editions. Sadly, all later revised and redrawn versions – initially re titled Norton’s 2000.0 and currently back to the original Norton’s Star Atlas – dropped these labels, to the dismay of observers. While this new atlas is primarily designed with observation of star clusters, nebulae, and galaxies in mind, it also serves as a general purpose guide for exploring all types of deep sky objects, showing as it does many prominent double and multiple stars, variable stars, asterisms, and the majestic Milky Way itself. Additionally, it may be viewed as a companion volume to our previous work, The Cambridge Double Star Atlas, first published in 2009. Between these two publications, the long standing lack of recognition accorded the discoveries of the Herschels, and those of the classic double star observers, by celestial cartographers has finally been rectified.

Who were the Herschels? Sir William Herschel William Herschel was without question the greatest visual observer who ever lived. Widely regarded as the “Father of Observational Astronomy,” he single handedly opened the frontiers of deep space to telescopic exploration. In the course of his grand scheme to study what he called the “construction of the heavens,” he discovered literally thousands of previously unknown double and multiple stars, star

clusters, nebulae, and what we know today as galaxies. Although self taught and so technically an amateur astronomer, he transformed the world of professional astronomy – which at the time had been largely concerned with the solar system and the positions of the stars. William was born into a musical family in Hanover, Germany, in 1739 and moved to England around 1770. Like others members of the family, his early career was that of a musician – in his case teaching and orchestrating music for the city of Bath. It was while there that he became fascinated with astronomy. (“Obsessed” would better describe it, for on occasions he would actually run home during performances to observe between acts! And later, as a full time astronomer, he typically observed from dusk to dawn.) He set about making his own telescopes beginning with small refractors but soon turned his attention instead to reflectors, constructing entire instruments, including their speculum metal mirrors, entirely himself. (The familiar metal on glass telescope mirror was not introduced until long after Herschel’s death in 1822.) But he not only became the greatest telescope maker of his day, he was also an observer the caliber of which the world had never seen before. He used these homemade instruments to “sweep” the heavens for unexplored celestial treasure, his initial “review” being undertaken with a “7 foot” Newtonian reflector at a magnification of 227
. (At that time telescopes were designated by their length rather than by their aperture.) This resulted in his first catalog of double and multiple stars. It also produced one of the greatest discoveries in the history of observational astronomy – made by a totally unknown “amateur”! While sweeping the sky in the constellation of Gemini on the night of March 13, 1781, Herschel came across a small greenish disk of light. Careful observation showed that it was slowly moving among the stars, leading him to believe that it was a

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The Cambridge Atlas of Herschel Objects

strange looking comet. Others agreed with him and for nearly a year mathematicians attempted to calculate an orbit on that basis. All attempts failed and it was finally realized that Herschel had, in fact, found another planet! This was the first such world ever discovered (the five naked eye planets having been known since antiquity) and it effectively doubled the size of the solar system. It apparently had never entered anyone’s mind that there actually could be more planets lying beyond those already known. This electrifying and unprecedented discovery catapulted William Herschel to instant fame and brought him to the attention of King George III, who appointed him his private astronomer. This honor brought with it a salary sufficient to allow Herschel to give up his musical duties and spend all his time on astronomy.

Caroline Herschel Any account of the work of William Herschel would be incomplete without mention of his devoted sister, Caroline Herschel. She assisted him both at the telescope at night and in the arduous work of recording and reducing his many discoveries in preparation for their eventual publication. This was in addition to taking care of household duties including meals (even mouth feeding and reading to her brother as he polished his mirrors for hours on end!). She became the leading woman astronomer of her day and the first to find a comet, her record of eight discoveries having stood for nearly two centuries. She observed with a small 27 inch focus Newtonian “comet sweeper” made expressly for her by William, using it to scan the sky on her own when he was away at meetings or showing the stars to the King and his court. Thus, a number of her own deep sky discoveries are contained in Sir William’s catalog. One of the author’s personal favorites is the lovely rich open cluster designated H VI 30 (or NGC 7789) in Cassiopeia, which the author named “Caroline’s Cluster” many years ago in her honor.

Sir John Herschel William Herschel married late in life, having a son named John Frederick William, or “John” for short. Like his father and his Aunt Caroline, John Herschel

also became famous as an astronomer. But in addition he was a gifted mathematician and scientist in other fields; among other activities he experimented with photography and took the oldest existing photograph on a glass plate (a ghostly image of his father’s 40 foot telescope). John is best known for completing his father’s survey of the northern sky and (especially) then extending it to the southern sky as well. He spent four years sweeping the heavens from Cape Town, South Africa, having taken his father’s favorite telescope – the “Large” 20 foot reflector – there and discovering thousands of previously unknown double stars, clusters, and nebulae. He returned to England in 1838 a national hero for this work, receiving among many other honors knighthood. John issued a compendium of his findings titled The General Catalog of Nebulae, and later a combined one containing all of his and his father’s telescopic discoveries totaling some 5,000 in all (including a few by other observers). This work eventually became the basis for the famed New General Catalogue of Nebulae and Clusters of Stars (or NGC), which was published in 1888. Only a hint can be gleaned of the incredible life and works of this remarkable family of astronomers from the brief account given here. Those desiring to know more about the Herschels are strongly encouraged to consult the various references given below, which make fascinating reading – especially on cloudy nights!

The Herschels’ telescopes Early instruments It will be instructive to say something about the telescopes the Herschels used to make their discoveries and to compare their performance with modern instruments. William Herschel began his telescope making career in 1773 by experimenting with relatively small refractors. But as these were then still optically primitive compared with today’s glasses, he soon turned his attention to reflectors. These could be made in larger sizes and without concern for the quality of optical glass, for they used mirrors instead of lenses. But these weren’t the familiar telescope mirrors of today, as metal on glass

The Herschels’ telescopes

optics did not appear until long after Herschel’s death. Instead, they were made of speculum metal – a hard brittle casting composed mainly of copper and tin. Herschel first made several mirrors for a 5.5 foot Gregorian reflector, but then turned to the simpler Newtonian form. All of his telescopes from that point on were long focus Newtonians of ever increasing size, culminating in the great 40 foot reflector (see below). He soon produced a 7 foot reflector, probably with an aperture of around 6 inches. He also made several 9 inch mirrors for a 10 foot reflector (and much later a 10 foot with a 24 inch mirror), followed by 20 foot models with 12 and 18.7 inch mirrors as described below. But his favorite early reflector was another 7 foot which contained “a most capital speculum” as he described it, of 6.2 inches aperture. This is the telescope that he used for his first “review” of the heavens and the one with which he discovered the planet Uranus. While most of the objects Herschel found in this first review with his prized 7 footer were double and multiple stars, he also found a number of his early clusters and nebulae with it. (It should be mentioned here that in his day, and long thereafter, galaxies were not yet recognized as such, being simply lumped under the category of “nebulae”.)

The 20-foot telescopes Herschel’s two “workhorse” telescopes – those used for all his later various reviews of the heavens – were his 20 foot reflectors. The earlier and smaller of these in terms of aperture (referred to as the “Small 20 Foot”) used 12 inch aperture mirrors, while the larger and later instrument (called the “Large 20 Foot”) used 18.7 inch mirrors. Note that “mirrors” is plural, since several were needed for each telescope – the one that was currently in use, and at least one in the process of being repolished and refigured because of the rapidity with which speculum metal tarnished! The 18.7 inch became Herschel’s most useful telescope and in later years he even preferred it to the massive 40 foot one, for it was both much easier to use and the mirrors performed better (not to mention that they were also vastly easier to make and keep ready). It was in constant use on clear nights from dusk to dawn,

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revealing over 2,000 previously unknown star clusters and nebulae. Owing to the huge light loss at each reflected surface of his reflectors, Herschel eventually decided to dispense with the secondary mirror in the Newtonian form. Instead, he tilted the primary mirror so that its focus could be examined off axis directly at the front of the tube – a form he referred to as the “front view.” This concept is still used in some amateur made telescopes today, but it’s now known as the “Herschelian” in honor of its inventor. And while loss of reflectivity is not the concern today that it was in Herschel’s time, moving the secondary mirror and its support out of the optical path essentially gives the unobstructed performance of a refractor combined with total freedom from the color aberrations inherent in lenses. It has frequently been stated that a modern 6 to 8 inch telescope will show a large percentage of the objects in the Herschel catalogs (including many of William’s faint and very faint nebulae), and that a good 12 inch should reveal every one of them even though most were found using the large 20 foot instrument. This is largely possible, of course, because of the much higher reflectivity of today’s coated glass telescope mirrors – and to a lesser extent because of modern eyepieces as well. (The Herschels primarily used single lens oculars; multiple element designs and antireflection coatings lay far in the future.) The author fully agrees with this assessment, based on half a century of viewing these wonders with telescopes of many different types ranging from 2 inches to 14 inches (and on occasion up to 30 inches – both reflectors and refractors) in aperture.

The great 40-foot telescope Sir William’s most ambitious telescope making project and, indeed, the most ambitious in history up to that time, was the construction of his “Great 40 Foot” reflector with its 48 inch mirror (or 4 feet in diameter, resulting in a focal ratio of f/10). He received financial support for this massive undertaking from the King, as well an annual allowance for upkeep of the telescope once it was completed. Herschel actually made several mirrors for it before he finally was able to get one that would take an acceptable polish and figure. In 1787, using

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The Cambridge Atlas of Herschel Objects

one of its first mirrors, Herschel climbed into the mouth of the huge tube and searched for the focus. His target was the Orion Nebula, which he described as “extremely bright” but the figure was far from perfect. On later attempts he used Saturn as his test object, discovering several new satellites while at it. Some idea of the light grasp of this instrument can be had from this famous account of the star Sirius as seen through it: . . . the appearance of Sirius announced itself, . . . and came on by degrees, increasing in brightness, till this brilliant star at last entered the field of view of the telescope, with all the splendour of the rising sun, and forced me to take the eye from that beautiful sight. Regular work with the telescope finally began in 1789. But Herschel was never pleased with the telescope’s performance. That very few of the objects contained in the Herschel catalogue were actually discovered with the 40 foot certainly confirms this statement. How very sad for Sir William after all his labors over this great instrument! But while it was a disappointment for him, it certainly was not for the many sightseers who came to gawk at this wonder of the ages, including royalty and dignitaries of all levels, and noted scientists from the world over. Even today, the image of Herschel’s mammoth 40 foot telescope remains one of the great – if not the greatest – icons of astronomical history, surpassed perhaps only by the Hubble Space Telescope itself. And here two very important facts need to be pointed out. First, all of Herschel’s many telescopes, including the 40 foot, were mounted as simple altazimuths, being moved about the sky and tracked manually. Secondly, they were all mounted outside of his various residences in the open night air. Amazingly, for all his fame and discoveries, Sir William never had an observatory!

The Herschel designations William Herschel’s classes Despite Sir William’s pioneering discoveries in the fields of solar system and stellar astronomy, it’s his deep space explorations for which he is best known and remembered. Some 2,500 star clusters and

nebulae (which included many galaxies, again the true nature of which was unrecognized at that time) were catalogued under the following eight categories, or “classes” as he called them, with the total number of objects in each indicated in parentheses: Class I – Bright Nebulae (288) Class II – Faint Nebulae (909) Class III – Very Faint Nebulae (984) Class IV – Planetary Nebulae (78) Class V – Very Large Nebulae (52) Class VI – Very Compressed and Rich Clusters of Stars (42) Class VII – Compressed Clusters of Small (Faint) and Large (Bright) Stars (67) Class VIII – Coarsely Scattered Clusters of Stars (88) Thus, William’s entire catalogue contains a total of 2,508 entries, with Classes II and III accounting for 1,893 of them. (Note that the actual number of objects is somewhat less than this, since some three dozen were either inexplicably assigned to more than one class or were entered twice in the same class.) Such a large number of targets (with a great percentage of them being labeled faint and very faint by their discoverer, who used the largest telescopes in the world at the time to find them) has discouraged many observers from attempting to view the entire catalog. The author suggested some years ago in both Sky & Telescope and Astronomy magazines that a much more realistic goal could be had by dropping Classes II and III as largely difficult and visually less interesting specimens, and going after the remaining 615 objects. This suggestion was the motivation for the founding of a national Herschel Club in the United States under the auspices of the Astronomical League (see the reference section on pages 42–3 for more about this). Out of respect for Messier’s work, William Herschel included relatively few of the famed “M objects” in his own compilations. Those he did include refer to features within those objects apparently unnoticed by Messier, as well as two of the infamous “missing” M objects (M 47 and M 48). Also included were the ones numbered from M 104 to M 110. These objects were only attributed to Messier long after Herschel’s time, later historical

The Herschel designations

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research showing that they had indeed been seen by Messier (or one of his colleagues) but were not included in his original catalog. In Sir John’s case, he did assign his own numbers to most of the Messier objects, as can be seen from the target list in Appendix B. Some may wonder why he included so many of Messier’s discoveries along with his own. Noted astronomical historian Michael Hoskin explains it this way: “John was preparing a catalogue of clusters and nebulae for efficient use by observers and it would have been bizarre to omit the most prominent [of them]. William, by contrast, was acting the natural historian and offering new specimens he had collected.” It should be noted that none of William Herschel’s objects will be found below a declination of about 33 degrees owing to the rather high latitude of his various observing sites around London. Had he been able to see even another 7 to 10 degrees further south, he would surely have laid claim to (and been thrilled by!) such wonders as the big, bright galaxies NGC 1316 and NGC 1365 in Fornax, and NGC 55 and NGC 300 in Sculptor; or the radiantly glorious open cluster NGC 2477 in Puppis; or the fascinating planetary NGC 3132 in Vela (the Eight Burst Planetary – rival of the northern sky’s famed Ring Nebula in Lyra). Instead, these were left to his son to find during his later survey of the southern sky. John did not use specific classes in his catalog of discoveries as his father had but a running number instead. (He also sometimes unintentionally gave two different numbers to the same object on different occasions.) Under the “Name/Notes” column in the target list in Appendix B, numbers are also given by John for many of William’s objects, these being the ones he assigned during his re survey of his father’s discoveries. Note also those objects designated in that column by “CH.” These are ones originally discovered by Caroline Herschel and later included in her brother’s catalog.

position), there’s the case of objects the Herschels discovered and catalogued but which supposedly can’t be found in the sky today! Many of these “disappearances” have involved entries in William’s Class VIII, which are coarsely scattered clusters of stars that were described as “poor” by him. As such, they are often difficult to pick out from the stellar background since most open clusters lie along the plane of the Milky Way’s rich stratum of stars. The modern story of Herschel objects apparently having vanished from the sky really dates back to 1973 when The Revised New General Catalogue of Nonstellar Astronomical Objects (or RNGC) was published by astronomers Jack Sulentic and William Tifft. The primary reference for this comprehensive work was photographs taken for the famed National Geographical Society–Palomar Observatory Sky Survey with the 48 inch Schmidt camera on Palomar Mountain, home of the 200 inch Hale reflector. Objects that could not be identified on the large scale plate prints were given a “type” code of “7” in the RNGC, meaning they are “nonexistent.” (They are indicated for objects in the Appendix B target list by “NE” under “Type.”) These included no fewer than 30 of the 88 clusters in William Herschel’s Class VIII alone. As a point of interest, it should be mentioned here that the RNGC compilers also rejected a number of John Herschel’s clusters as not existing in addition to those of his father. In 1975 two Canadian amateur astronomers – Patrick Brennan and David Ambrosi – began examining the sky for these missing objects using a modest 6 inch reflector. As Brennan later wrote, “Have you ever encountered a ‘nonexistent’ RNGC cluster alive and well, so to speak?” These observers found that many of the rejected Herschel clusters actually were visible in the eyepiece even if they weren’t distinguishable on the Palomar prints, and so were not really missing after all. Based on the author’s personal experience, most of the missing Herschel objects do, in fact, exist and offer observers a wonderful challenge to identify them.

“Nonexistent” objects

Miscataloged objects

In a situation analogous to the saga of the famed “missing” Messier objects (which have now all been accounted for as errors in identification and/or

A fair number of William Herschel’s discoveries were cataloged in the wrong class (and to a lesser extent those of John as well). As just one striking example,

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The Cambridge Atlas of Herschel Objects

there’s H IV 50 (NGC 6229) in Hercules. William considered this little object to be a planetary nebula and so it was long viewed to be such by most of the classic observers. And indeed, it does look like a typical planetary in the eyepiece. But, in reality, it’s a globular cluster that apparently was beyond the resolution capabilities of his telescopes. And many other small globular clusters were assigned to Class I as nebulae. (In John’s case, a number of objects listed by him as globulars are in reality tight open clusters.) Likewise, Class IV actually contains many diffuse nebulae and more galaxies than true planetaries! Such misidentifications as these are hardly unexpected, for nothing was known at the time of the actual physical nature of most of the nebulous objects seen in the eyepiece, spectroscopic analysis and astrophysics still lying in the future. The Herschels based the classification of their discoveries solely upon their visual appearance in their various telescopes. But all of this adds to the fascination of viewing these objects, as we attempt to verify their eyepiece impressions and to see why the Herschels placed them in the classes they did. And, while having to rely strictly on what these objects looked like to the eye resulted in a sizeable number of objects being misclassified, in other cases this reliance led to some profound insights and discoveries. One example with important historical significance involves the planetary nebula H IV 69 (NGC 1514) in Taurus, which appears as an obvious nebulous halo surrounding a 9th magnitude star even in small telescopes. Here is Sir William’s description of this object: “A most singular phenomenon! A star of about 8th magnitude with a faint luminous atmosphere, of circular form, and about 3 minutes in diameter. The star is in the centre, and the atmosphere is so faint and delicate and equal throughout that there can be no surmise of it consisting of stars; nor can there be a doubt of the evident connexion between the atmosphere and the star.” Thus he recognized for the first time the existence of “a shining fluid of a nature totally unknown to us” as he described it. Until this observation, all diffuse nebulae were thought to be simply unresolved masses of stars. This amazing deduction – based solely on the appearance of this object

in the eyepiece of the telescope – showed nebulae to be gaseous long before the spectroscope actually proved it! Such is the power of really seeing what it is you are looking at in the eyepiece, as Sir William himself advised. Finally, mention should be made that William Herschel’s various discoveries originally appeared as papers in the Philosophical Transactions of the Royal Society of London in the late 1700s. In 1864, John Herschel published his monumental General Catalogue of Nebulae (or GC) also in the Transactions, its more than 5,000 entries having been found mostly by his father and himself. Based heavily on the GC, J.L.E. Dreyer subsequently compiled the famed New General Catalogue of Nebulae and Clusters of Stars (or NGC). Its 7,840 entries contain among them the only complete listing of all of Sir William’s and Sir John’s discoveries outside of the GC itself, providing shorthand descriptive notations that they invented. These were adopted by Dreyer, and in some cases added to in the light of more recent (at that time) knowledge.

Overlooked objects As thoroughly as the three Herschels swept the skies (especially those visible from England), they still inexplicably missed a number of fascinating objects – all of which are visible in typical backyard telescopes today. Among these are the Helix Nebula in Aquarius, the Flaming Star Nebula in Auriga, Stephan’s/Webb’s Protoplanetary Nebula in Cygnus (which rivals the famed Blinking Planetary also in Cygnus – so named by the author in 1963 from its amazing behavior – which Sir William did discover), Barnard’s Dwarf Galaxy in Sagittarius, and Hind’s Variable Nebula in Taurus. One of the author’s favorite overlooked objects is the big but dim open cluster NGC 6791 in Lyra. This amazingly rich swarm hosts over 300 stars and looks very much like a globular cluster, both visually and on photographs.

Map parameters and selection criteria The 32 maps comprising this Atlas were planned, drawn and labeled by Wil Tirion, widely recognized as the world’s greatest celestial “cartographer” and creator of such classic works as the magnificent Sky Atlas 2000.0 and The Cambridge Double Star Atlas.

Instrumental factors

They show over 2,500 of the brighter Herschel objects suitable for viewing with typical backyard telescopes in the 2 inch to 14 inch aperture range. In addition to this introductory guide to the Atlas, the original target list in Appendix B and the showpiece roster below were compiled by James Mullaney based on his personal observations of thousands of Herschel objects over the past 50 years – ones using literally hundreds of telescopes of all types and sizes within the aperture range stated above. No doubt experienced observers will have favorites that are not shown, but those that are certainly include the best of the Herschels’ discoveries. (All 400 objects on the Astronomical League’s Herschel 400 Club target list are also included, being designated with an asterisk there.) All told, some 25,000 stars are plotted in half magnitude steps on the maps to a visual magnitude limit of 7.5. The nominal visual magnitude cutoff for the Herschel objects themselves is 12.5. However, some fainter ones are included that have special appeal. In the case of Classes I, IV, V, VI, VII, and VIII, every object in each class, whatever its magnitude, is shown in order to provide observers with the complete contents of these six visually rewarding groups (those suggested by the author as the basis for creating Herschel clubs). Note that all of William Herschel’s objects appear on the maps without an “H” prefix (since his classes clearly identify his discoveries), while John Herschel’s have an “h” prefix. And while mentioning dim objects below the map limit, it’s very important to point out here that many of the Herschel objects plotted often have one or more fainter objects lying within the same wide, low-power eyepiece field (ones found by the Herschels and by others)! Thus, the field of view should always be scrutinized for these in addition to the primary target itself. A magnitude scale and color coded key to the symbols used to denote various types of deep sky objects appear at the top of each map. Note that the edges of the maps have blue arrowed numbers indicating adjoining ones (with some overlap) in each direction, which will be found very helpful in navigating the Atlas. Also, soft lavender lines have been used to connect the principal stars in each constellation, the boundaries of which are indicated

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by dashed lavender lines. (Note that all of the lines used are “red light friendly,” remaining visible when employing such illumination to preserve night vision.) These so called “stick figures” also aid in finding your way around the sky. Many observers today use computerized (“Go To”) target acquisition, and most of the brighter Herschels plotted on the maps – particularly those given in the showpiece roster below – can be located by entering their NGC designation, common name and/or coordinates on the controller’s keypad. (Again, see Appendix B for data on all objects plotted.) To many of us “purists,” this modern technology takes away much of the fun of good old fashioned “star hopping” (or “sweeping” as the Herschels did) to learn and find your way around the sky – which is really one of the primary purposes of a star atlas like this and one of the joys of leisurely stargazing!

Instrumental factors Light-grasp, resolution and magnification There are three types of “power” used in describing a telescope’s capabilities. The one uppermost in most beginners’ minds is magnification, but it is actually the least important of the three. The primary one for viewing the Herschel objects (the majority of which are faint compared with other types of celestial objects) is its light-gathering power. Simply stated, the larger the telescope, the more light it collects and the brighter the image it delivers. And it’s paramount here to realize that doubling the aperture of a telescope quadruples the amount of light collected, since the area of the objective lens or primary mirror increases as the square of its diameter. Next in importance is the telescope’s resolving power, or ability to reveal fine detail in an image. Much has been written in the literature over the years about the resolution capabilities of various apertures, particularly in regards to the splitting of close double stars. The best known and most widely used of the various resolution criteria is the famed Dawes’ Limit, R ¼ 4.56/A, where R is the resolution in arc seconds and A is the telescope’s aperture in inches. (For much more about this see the introductory section of The Cambridge Double Star Atlas.) The primary factor at

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The Cambridge Atlas of Herschel Objects

play in determining if a given telescope will resolve tight clusters, or show structure in a nebula or galaxy (aside from atmospheric conditions) is aperture. And in this case, when the aperture is doubled, so too is the resolution – a telescope twice as big as another one will show twice as much detail (assuming they are both of the same optical quality). In achieving optimum results here (particularly in the case of resolving fine planetary detail or splitting close double stars), the telescope should be used at what is known as its “resolving magnification.” This is typically given as 25
per inch of aperture, which leads us to a telescope’s magnifying power, or how many times bigger it makes an object than what the unaided eye sees. Observers typically employ a range of low, medium, and high powers on their instruments. Recommended magnifications for viewing a Herschel object depend on what type it is. For big scattered open clusters or extensive nebulosities (and even a few of the largest galaxies), the lowest possible power and widest field of view (which depends on eyepiece design) give the most pleasing results. The same applies in the initial sweeping for objects to find them. In the case of rich, compact open clusters and tight globulars, medium magnifications typically give the best view. The same goes for the smaller diffuse nebulae and most planetaries, and also for galaxies in general. Unless the atmosphere is steady, high powers can give a “washed out” appearance to the image and typically greatly restrict the field of view. But they are still worth trying on all but the very largest of objects to see if any additional details are revealed. Another factor affecting telescopic image quality aside from atmospheric conditions (see below) is that known as “local seeing” or the thermal conditions in and around the telescope itself. Heat radiating from driveways, walks and streets, houses and other structures (especially on nights following hot days) plays a significant role. This is why observing from grassy areas away from buildings gives the best results. The cooling of the telescope’s optics and tube assembly is especially critical to achieving sharp images. Depending on the season of the year, it may take up to an hour or more for the optics (especially the primary mirror in larger reflectors) to reach

equilibrium with the cooling night air. During this cool down process, air currents within the telescope tube itself can play absolute havoc with image quality, no matter how good the optics and atmospheric seeing are. (This is less of a concern using refractors with their closed tubes, which in smaller apertures at least are essentially ready for immediate use.) Surprisingly, even the heat radiating from the observer’s body can be a factor here if concerned with optimum resolution, particularly with reflecting telescopes having open tubed truss style designs. For much more on all aspects of telescopes and their use, see A Buyer’s and User’s Guide to Astronomical Telescopes and Binoculars, by the author (Springer Verlag, London, 2007).

Optical quality and collimation For the casual observation of the Moon, planets and brighter deep sky wonders, a telescope of even mediocre optical quality can provide acceptable views. But for optimum viewing, good to excellent optical quality is essential. The condition of a telescope’s optics and its all important optical alignment can readily be determined by a simple test using a star itself. Known as the extrafocal image test, this involves looking at the image of a star, both inside and outside of focus, using a medium to high power eyepiece. An ideal target for this purpose is Polaris in Ursa Minor (the Pole Star), which is neither too bright nor too faint, and has the great added advantage of not moving in the eyepiece as the Earth rotates, in case your instrument isn’t motorized! A telescope having first class (or “diffraction limited”) optics in perfect alignment (or collimation – see below) will show identical circular disks of light with a pattern of faint concentric interference rings on either side of focus as the eyepiece is racked in and out. These rings should be uniformly spaced and of even intensity. If not, this indicates zones in the optical figure – a condition known as “spherical aberration.” A “shaggy” look to the rings indicates a rough polish to the glass rather than the desired smooth one. If the extrafocal images are triangular rather than circular, this shows that the objective lens or mirror is pinched in its cell. Elliptical shaped images that rotate 90 degrees on

Observing hints

either side of focus are the most to be feared, since they reveal the serious optical defect known as “astigmatism” or a warping of the glass itself. However, astigmatism in the observer’s own eye, a bad eyepiece, and especially optical misalignment can each produce the same effect! Optical collimation is an entire subject unto itself. The term describes that condition in which all of the optical elements in a telescope are precisely lined up on the same optical axis – something that can be achieved by examining the extrafocal image (among other methods) while adjusting the alignment. The need for and actual process of collimation depends upon the type of instrument being used. Refractors and Maksutov–Cassegrains are typically permanently collimated, and in many cases no provision is even made for adjustment. Reflectors and Schmidt– Cassegrains typically do require periodic collimation, instructions for which are normally included in the manuals provided with commercially made telescopes. For optimum resolution and image contrast, a precisely collimated telescope is an absolute must. (The ultimate reference on interpreting extrafocal images and testing/ collimating telescope optics is Harold Richard Suiter’s Star Testing Astronomical Telescopes: A Manual for Optical Evaluation and Adjustment, Willmann Bell, Inc., Richmond VA, 2009.) And one final note here: the extrafocal image test also makes it possible to judge something of the seeing conditions, ranging from local conditions within and immediately above the telescope to the upper atmosphere itself. Undulating waves and flashing patterns of light crossing over the image can say much about the steadiness of the atmosphere, as well as the telescope’s thermal state and environment. Careful focusing will reveal moving patterns seemingly “floating” at different levels above the light path and (with experience) show if disturbances are atmospheric, or are within the telescope itself or its immediate vicinity.

Observing hints It’s often claimed that the person behind the eyepiece of a telescope is far more important than the size or type or quality of the instrument itself. The truth of

9

this adage has proven itself time and again. Typical examples are that of a skilled observer using a small telescope seeing intricate detail on a planet like Jupiter or Mars at opposition, or subtle structure in a nebula or galaxy, that completely escapes an inexperienced observer using a much larger aperture. The fact is that the eye does not work alone, but in conjunction with the most marvelous “image processor” known – the human brain! It was Sir William Herschel himself, the greatest visual observer of all time, who said that “seeing” is an art and that as observers we must properly educate our eyes to really see what it is we are looking at in the eyepiece. And so this section is aimed at helping you get the most out of your nightly explorations of the heavens – especially in the observation of the star clusters, nebulae and galaxies discovered by the Herschels.

Training the eye There are several distinct areas in which the human eye/brain combination can be “educated” to see better. We begin with two of especial importance when it comes to looking at Herschel objects. The first involves the technique of using averted (or side) vision in viewing faint deep sky targets. This makes use of the well known fact that the outer portion of the retina of the eye – that containing the receptors called rods – is much more sensitive to low levels of illumination than is the center of the eye containing the receptors known as cones. (See the discussion below on color perception.) This explains the common experience when driving at night of objects seen out of the corner of your eye appearing brighter than they actually are if you turn and look directly at them. Averted vision is especially useful in viewing low surface brightness targets like nebulae and galaxies, where the increase in the apparent brightness of the image is typically more than doubled. The second area is that of dark adaptation. It’s an obvious fact that the eyes needs time to adjust to the dark after coming out of a brightly lit room. Two factors are at play here. One is the dilation of the pupils themselves, which begins immediately upon entering the dark and continues for several minutes. The other involves the actual chemistry of the eye,

10

The Cambridge Atlas of Herschel Objects

as the hormone rhodopsin (often called “visual purple”) stimulates the sensitivity of the rods to low levels of illumination. The combined result is that night vision improves noticeably for perhaps half an hour or so, continuing slowly thereafter. This explains why the sky looks black on first going outside, but later appears gray as you fully adjust to the dark. In the first instance, it’s a contrast effect and in the second the eye has become sensitive to stray light, light pollution, and the natural airglow of the sky itself that were not seen initially. White lighting causes the eye to lose its sensitivity while red light preserves it, which is the reason for the well known standard practice of using red illumination for reading star maps and making notes at the eyepiece. Another aspect of training the eye is that of visual acuity – the ability to see or resolve fine detail in an image or in splitting close double stars. There’s no question that the more time you spend at the eyepiece, the more detail you will eventually see. Even without any real purposeful training plan in mind, the eye/brain combination will learn to search for and find ever finer detail in what it is viewing. But this process can be considerably accelerated by a simple exercise repeated daily for a period of several weeks. On a piece of white paper, draw a circle about 3 inches in diameter. Then using a soft pencil, randomly place various markings within the circle, ranging from broad patchy shadings to fine lines and points. Now place the paper at the opposite side of a room at least 20 feet or so away, and begin drawing what you see using the unaided eye. Initially, only the larger markings will be evident, but as you repeat this process over a period of time, more and more of the markings will become visible to you. Tests have shown improvements in overall visual acuity by as much as a factor of 10 from using such a procedure! A final important area involving the eye/brain combination is that of color perception. At first glance, to the unaided eye the stars all appear to be white. But, upon closer inspection, differences in tint among the brighter ones reveal themselves. The lovely contrasting hues of ruddy orange Betelgeuse and blue white Rigel in the constellation of Orion is one striking example visible in the evening sky around

January and February. Another can be found by comparing blue white Vega in Lyra, orange Arcturus in Bootes and ruddy Antares in Scorpius – seen best together in the evening sky in July. Indeed, the sky is alive with color once you’ve been trained to see it! While the rods in the edge of the eye are light sensitive, they are essentially colorblind. Thus, for viewing the tints of stars in the more prominent open clusters, the subtle coloration of the brighter diffuse nebulae, and the eerie unearthly tints of many of the planetaries, direct vision should be employed – making use of the color sensitive cones at the center of the eye. In short, stare directly at an object to perceive its color and off to the side to see it brighter.

Sky conditions A number of atmospheric and related factors affect the visibility and appearance of celestial objects in the telescope. In the case of resolving tight open clusters or compact globulars, or seeing detail within nebulae or galaxies, the most important of these is atmospheric turbulence or seeing, which is an indication of the steadiness of the image. On some nights, the air is so unsteady (or “boiling” as it’s sometimes referred to) that star images appear as big puffy, shimmering balls, and detail on the Moon and planets is all but nonexistent. This typically happens on nights of high transparency – those having crystal clear skies in which the air overhead is in a state of rapid motion and agitation. These nights are ideal for viewing faint objects like nebulae and remote galaxies. On other nights, fine detail stands out on the Moon and planets like an artist’s etching and star images are nearly pinpoints showing virtually no motion. Such nights are often hazy and/ or muggy, indicating stagnant tranquil air over the observer’s head, making them poor for viewing “faint fuzzies.” Occasionally, observers are blessed with nights of both good seeing and transparency (such as those typically found at many of the world’s major mountaintop observatories). Such opportunities should be utilized to the fullest and often result in “all nighters” in which observing sessions begin after sunset and continue until dawn! Various “seeing scales” are employed by observers to quantify the

Observing hints

state of atmospheric steadiness and transparency. One of the most common of these uses a 1 to 5 numerical scale, with 1 indicating poor, 3 average, and 5 excellent conditions. Others employ a 1 to 10 system, with 1 again representing very poor and 10 representing virtually perfect sky conditions. (In some schemes, the numerical sequence is reversed, with lower numbers indicating better and higher numbers poorer conditions.) Casual observing can usually be done on all but the worst of nights (which includes those around the time of the Full Moon when the sky is flooded with light), but optimum views of the Herschel objects (especially the fainter ones) demand excellent conditions.

Record-keeping From a strictly personal perspective, an account of what has been seen during your nightly vigils under the stars can have a wonderful impact as you look back over the years at the first views of particular Herschel objects (or celestial wonders in general). Your eyepiece impressions recorded on paper (written and/or sketched) or perhaps audio taped can provide many hours of nostalgic pleasure in years to come. For casual deep sky observing in particular, there’s definite aesthetic value in logging the various objects seen (especially the showpiece ones!), including the degree of visibility in a given telescope at a particular magnification under various sky conditions. In the case of those desiring a coveted Astronomical League Herschel 400 Club Certificate for observing all the entries on its target list (which are indicated with asterisks in Appendix B), you must submit documentation along the following lines. The information in your logbook should ideally include: the date, and beginning and end times of your observations (preferably Universal Time/Date); telescope size, type and brand used; magnification/s employed; sky conditions (seeing and transparency, along with notes on passing clouds, wind, haze, moonlight and other sources of light pollution); and finally a brief description of each object seen. And here, despite its ultimate value, it’s strongly advised to keep your journaling as brief as

11

possible. Some observers spend far more time writing about the wonders they see at the eyepiece than they actually do viewing them!

Personal considerations There are a number of little recognized factors that affect the enjoyment and success of an observing session at the telescope, one of which concerns proper dress. This is of particular importance in the cold winter months of the year, when sub freezing temperatures are often experienced at night. It’s impossible to be effective at the eyepiece, or even to just appreciate the views, when you’re half frozen to death! Proper protection of the head, hands and feet are especially important during such times, and several layers of clothing are recommended as opposed to one heavy one for thermal insulation of the body in general. During the summer months, the opposite problem occurs as observers attempt to stay cool. And, in addition to very short nights at this time of year, there’s the added annoyance of flying insects and optics fogging humidity and dew. Another concern is proper posture at the telescope. It’s been repeatedly shown that the eye sees more detail in a comfortably seated position than when standing, twisting or bending at the eyepiece! If you must stand, be sure that the eyepiece/focuser is at a level and position where you don’t have to strain your neck and head to look into it. And, while not as critical, the same goes for positioning finder scopes where they can be reached without undue contortions. Finally, proper rest and diet both play a role in experiencing a pleasurable observing session. Attempting to stargaze when you’re physically and/ or mentally exhausted is guaranteed to leave you frustrated. Even a brief nap before going out to observe after a hectic day is a real help here. Heavy meals can make you feel sluggish and unable to function alertly at the telescope. It’s much better to “refuel” after you’re done stargazing – especially since most observers find themselves famished then (particularly on cold nights). Various liquid refreshments such as tea, coffee and hot chocolate can provide a needed energy boost while observing (and warmth when desired).

12

The Cambridge Atlas of Herschel Objects

We conclude this section on an aesthetic and philosophical note. There’s no question that the more you know about the wonders revealed by a telescope the more meaning they will hold for you. Realizing in the case of the Herschel objects that the stellar beehive you’re viewing contains upwards of a million suns and that the light you see it by left there 25,000 years ago when cavemen were still hunting mastodons certainly adds to the thrill of the view. So too does that misty gossamer patch of light in the eyepiece when you know it represents a stellar nursery where new stars (and their planets) are forming right before your eyes, or in other cases involving small spheroids and ellipsoids when you are witnessing the death throes of a dying sun. The ultimate example of this process of “seeing with your mind as well as sight” involves galaxies. That dimly perceived elongated glow in the eyepiece may contain as many as half a trillion stars, and the light you’re seeing from them left there millions of years ago while the dinosaurs were roaming the Earth. You are getting archaic photons that were once inside of these vast star cities inside of you ending their long journey through space and time on the retina of your eye (an experience the author calls “making the photon connection”)! This matter of preparedness before going to the telescope has likely never been more eloquently expressed than in the following lines from Charles Edward Barns’ 1929 classic work, 1001 Celestial Wonders: Let me learn all that is known of them, Love them for the joy of loving. For, as a traveler in far countries Brings back only what he takes, So shall the scope of my foreknowledge Measure the depth of their profit and charm to me. Lo, the Star-lords are assembling, And the banquet-board is set; We approach with fear and trembling, But we leave them with regret.

Herschel showpieces Following is a sampling of 215 of the best Herschel objects shown in this Atlas for viewing with telescopes from 2 inches to 14 inches in aperture.

Many of these can be seen in the smallest of glasses, and some of them even in binoculars. Arranged in order of increasing Right Ascension, the first column (Herschel) gives the class and number from Sir William’s catalog, or Sir John’s catalog number. The next one shows the New General Catalogue number, plus Messier designation if any (NGC/M). Constellation (Con) abbreviations are the official three letter ones adopted by the International Astronomical Union (see Appendix A). Right Ascension (RA) in hours and minutes, and Declination (Dec) in degrees and minutes, are for the current standard Epoch 2000.0. Other headings are the apparent visual magnitude (Mag) and apparent angular size in arc minutes (Size). The object’s actual class or type (Type) is indicated using the following abbreviations: OC open cluster, GC globular cluster, PN planetary nebula, DN diffuse nebula, SR supernova remnant, GX galaxy, NE “nonexistent.” Note that this may differ in many cases from what the Herschels assigned to it and that galaxies were not recognized as such in their time. Map number (Map no.) indicates those on which the object is plotted on the charts in this Atlas. In the case of those numbers shown in italics, the object is plotted but unlabeled, being covered by the two larger scale maps. (Name/Notes) gives the popular name/s (if any), comments by the author, and the NGC description in italics based primarily on Sir William’s or Sir John’s eyepiece impressions. Note that the magnitudes stated in these descriptions often depart markedly from modern values, especially in the case of the fainter stars in clusters. “CH” indicates one of the objects originally discovered by Caroline Herschel. The approximate distance in light years (LY) is also given in many cases. Primary data sources used were the same ones as those listed in the header for the target list in Appendix B. Not only does this roster provide a great sampling of Herschel wonders in itself, but it also serves as ideal preparation for those observers who may be considering viewing as many as possible of the 2,500 plus objects shown in the Atlas visible from their latitude.

13

55

104

129

185

205/M 110

225

246

247

188

h 2315

h 2322

H VIII-79

H II-707

H V-18

H VIII-78

H V-25

H V-20

h 34

253

40

H IV-58

H V-1

NGC/M

Herschel

RA (2000.0)

Dec

SCL 00 47.6 25 17 Remarkable, very much so, very very bright, very very large, very much extended 54 degrees, gradually brighter in the middle.

CEP 00 47.5 þ85 20 Cluster, very large, round, 150 to 200 stars of magnitude 10 to 18.

CET 00 47.1 20 46 Faint, extremely large, very much extended 172 degrees.

CET 00.47.0 11 53 Very faint, large, 4 stars in diffused nebula.

CAS 00 43.4 þ61 47 Cluster, large, little compressed, stars of magnitude 9 to 10.

AND 00 40.4 þ41 41 Very bright, very large, much extended 165 degrees, very gradually very much brighter in the middle.

CAS 00 39.0 þ48 20 Very bright, very large, irregularly round, very gradually much brighter in the middle, resolvable (mottled, not resolved).

CAS 00 29.9 þ60 14 Cluster, very large, pretty round, little compressed, stars of magnitude 9 to 13.

TUC 00 24.1 72 05 Globular cluster, remarkable, very much so, very bright, very large, very much compressed in the middle.

SCL 00 14.9 39 11 Very bright, very large, very much extended, trinuclear.

CEP 00 13.0 þ72 32 Faint, very small, round, very suddenly much brighter in the middle, a star of 12th magnitude south preceding.

Con

Herschel showpieces

GX

OC

GX

PN

OC

GX

GX

OC

GC

GX

PN

Type

Size

7.3

8.1

8.9

10.9

7.0

7.9

9.3

6.5

4.0

7.8

2, 6

2

19.50
11.50 Dim companion to Andromeda Galaxy (M 31), CH 9 2,900,000 LY Sailboat Cluster, CH 11 C 15 2,100 LY 1,600 LY

15.00

4.10

1 The Ancient One (12 billion years old!). 5,000 LY Sculptor Galaxy, CH 10 Big, bright and bold! 10,000,000 LY

15.00

29.00
6.80

2

20

19.20
5.50

12, 20

2, 6

2,300,000 LY

8.00
7.00

26, 30

2

47 Tucanae Cluster Magnificent stellar beehive! 13,400 LY

31.00

20

1, 2

Map no.

21.00

7,000,000 LY

Magnitude very uncertain – seems much brighter (10.2?). 3,000 LY

Name/Notes

31.20
5.90

12.3? 1.20

Mag

14

292

300

362

404

457

598/M 33

604

651þ650/ M 76

654

663

752

h 2359

h 2375

H II-224

H VII-42

H V-17

H III-150

H I-193

H VII-46

H VI-31

H VII-32

288

H VI-20

h 2356

NGC/M

Herschel

RA (2000.0)

Dec

þ51 35

AND 01 57.8 þ37 41 Cluster, very very large, rich in stars, stars large [bright] and scattered.

CAS 01 46.0 þ61 15 Cluster, bright, large, extremely rich in stars, stars pretty large [bright].

CAS 01 44.1 þ61 53 Cluster, irregular figure, rich in stars, a single star of magnitude 6 or 8, stars of magnitude 11 to 14.

PER 01 42.3 Very bright, preceding double nebula.

TRI 01 34.5 þ30 48 Bright, very small, round, very very little brighter in the middle.

TRI 01 33.9 þ30 39 Remarkable, extremely bright, extremely large, round, very gradually brighter to a nucleus.

CAS 01 19.1 þ58 20 Cluster, bright, large, pretty rich in stars, stars of 7th, 8th, 10th magnitude.

AND 01 09.4 þ35 43 Pretty bright, considerably large, round, gradually brighter in the middle, Beta AND south following.

TUC 01 03.2 70 51 Globular cluster, very bright, very large, very compressed, very much brighter in the middle, stars of magnitude 13 to 14.

SCL 00 54.9 37 41 Pretty bright, very large, very much irregularly extended, very gradually pretty much brighter in the middle.

TUC 00 52.8 72 50 Cluster, faint [??], most extremely large, round, stars of magnitude 12 to 18.

SCL 00 52.8 26 35 Globular cluster, bright, large, little extended, stars of magnitude 12 to 16.

Con

OC

OC

OC

PN

DN

GX

OC

GX

GC

GX

GX

GC

Type

5.7

7.1

6.5

10.1

12.0

5.5

6.4

10.1

6.8

8.1

2.2

8.1

Mag

26, 30

28,000 LY

Mirach’s (Beta AND) Ghost/False Comet. 8,000,000 LY ET/Owl Cluster. 9,300 LY

14.00

3.50

20.00

Little Dumbbell/Barbell Nebula. 3,400 LY

1.10

2, 3

2, 3

2, 6, 7

6.00

15.00

75.00

CH 13 Wide matched double 56 AND on edge. 1,300 LY

6 Star formation region within the Triangulum Galaxy.

2.00

2

6

68.70
41.60 Triangulum Galaxy Huge but elusive star city! 3,000,000 LY

2, 3

6

20

26, 30

20

Map no.

19.00
12.90 8,000,000 LY

Small Magellanic Cloud Amazing naked-eye wonder! 210,000 LY

29,000 LY

13.00

3190
200

Name/Notes

Size

15

891

1023

1027

1097

1261

1245

1291

1313

1316

H V-19

H I-156

H VIII-66

H V-48

h 2517

H VI-25

h 2521

h 2528

h 2527

1342

884

H VI-34

H VIII-88

869

H VI-33

PER Cluster, very large, about 60 stars.

03 31.6

þ37 20

FOR 03 22.7 37 12 Very bright, considerably large, very little extended, very suddenly very much brighter in the middle to a nucleus.

RET 03 18.3 66 30 Pretty bright, large, extended, very gradually brighter in the middle, resolvable (mottled, not resolved).

ERI 03 17.3 41 08 Globular cluster, very bright, pretty large, round, much brighter in the middle, easily resolvable.

PER 03 14.7 þ47 15 Cluster, pretty large, rich in stars, compressed, irregularly round, stars of magnitude 12 to 15.

HOR 03 12.3 55 13 Globular cluster, bright, large, round, partially resolved, some stars seen.

FOR 02 46.3 30 17 Very bright, large, very much extended 151 degrees, very much brighter in the middle to a nucleus.

CAS 02 42.7 þ61 33 Cluster, large, scattered stars, one 10th magnitude.

PER 02 40.4 þ39 04 Very bright, very large, very much extended, very very much brighter in the middle.

AND 02 22.6 þ42 21 Remarkable, bright, very large, very much extended 22 degrees.

PER 02 22.4 þ57 07 Remarkable, cluster, very large, very rich in stars, ruby star in the middle.

PER 02 19.0 þ57 09 Remarkable, cluster, very very large, very rich in stars, stars of magnitude 7 to 14.

OC

GX

GX

GX

OC

GC

GX

OC

GX

GX

OC

OC

6.7

8.4

9.1

8.5

8.4

8.3

9.5

6.7

9.5

10.1

6.1

5.3

21

26, 27

54,000 LY

8,000 LY

9.40
6.60

6.80

10.00

Fornax A. 55,000,000 LY

11.00
7.20

17.00

26, 27, 30

15,000,000 LY

9.20
7.20

21

21

21

11.00
9.50

3, 7

2, 3

2, 6, 7

15.00

Was CH 9 (which is actually M 110 – see above). 10,000,000 LY

11.70
1.60

2, 3

7

Double Cluster. 7,100 LY Magnificent stellar jewelbox!

18.00

2, 3

7.40
2.50

Double Cluster. 7,100 LY Magnificent stellar jewelbox!

18.00

16

1407

1444

1501

1502

1514

1513

1535

1528

1545

1778

H VIII-80

H IV-53

H VII-47

H IV-69

H VII-60

H IV-26

H VII-61

H VIII-85

H VIII-61

1365

h 2552

H I-107

NGC/M

Herschel

RA (2000.0)

Dec

þ62 20

AUR 05 08.1 þ37 03 Cluster, pretty compressed, little rich in stars, irregular figure, stars large [bright].

PER 04 20.9 þ50 15 Cluster, pretty rich in stars, little compressed, stars large [bright].

PER 04 15.4 þ51 14 Cluster, bright, very rich in stars, considerably compressed.

ERI 04 14.2 12 44 Planetary nebula, very bright, small, round, very suddenly brighter in the middle, resolvable (mottled, not resolved).

PER 04 10.0 þ49 31 Cluster, large, very rich in stars, pretty compressed, stars very large [bright].

TAU 04 09.2 þ30 47 A star of 9th magnitude in nebula 30 in diameter.

CAM 04 07.7 Cluster, pretty rich in stars, considerably compressed, irregular figure.

CAM 04 07.0 þ60 55 Planetary nebula, pretty bright, pretty small, very little extended, 10 in diameter.

PER 03 49.4 þ52 40 Cluster of about 30 stars of magnitude 12 to 14.

ERI 03 40.2 18 35 Very bright, large, round, suddenly very much brighter in the middle to a nucleus.

FOR 03 33.6 36 08 Remarkable, very much so, very bright, very large, much extended, resolvable (mottled, not resolved) nucleus.

Con

OC

OC

OC

PN

OC

PN

OC

PN

OC

GX

GX

Type

7.7

6.2

6.4

9.6

8.4

10.9

6.9

11.5

6.6

9.7

9.5

Mag

Golden Harp Cluster 3,000 LY Crystal Ball Nebula. Historic planetary – see text.

20.00

2.20

3

3, 7

7

12.00

8.00

13, 14, 21

0.80

18.00

3, 7

7

12.00

Lassell’s Most Extraordinary Object. Distance unknown!

2, 3

Oyster Nebula

0.90

2, 3

3

4.00

21

13, 21

60,000,000 LY

11.00
6.20

Map no.

4.60
4.30

Name/Notes

Size

17

1850

1817

1851

1857

1981

1977

1982/M 43

2070

2017

2024

2022

h 2780

H VII-4

h 2777

H VII-33

h 362

H V-30

H III-1

h 2941

h 2896

H V-28

H IV-34

17 51

ORI 05 42.1 þ09 05 Planetary nebula, pretty bright, very small, very little extended.

ORI 05 41.9 01 51 Remarkable, irregular, bright, very very large, black space included.

LEP 05 39.4 Cluster of large [bright] stars.

DOR 05 38.6 69 05 A magnificent or otherwise interesting object, very bright, very large, looped.

ORI 05 35.6 05 16 Remarkable, very bright, very large, round with tail, much brighter in the middle, a star of magnitude 8 or 9.

ORI 05 35.5 04 52 Remarkable, very much so, 42 ORI and nebula.

ORI 05 35.2 04 26 Cluster, very bright, little rich in stars, stars large [bright], scattered.

AUR 05 20.2 þ39 21 Cluster, pretty rich in stars, pretty compressed, stars of 7th magnitude and fainter.

COL 05 14.1 40 03 Globular cluster, remarkable, very bright, very large, round, very suddenly very much brighter in the middle, well resolved, clearly consisting of stars.

TAU 05 12.1 þ16 42 Cluster, large, rich in stars, little compressed, stars of magnitude 11 to 14.

DOR 05 08.5 68 46 Globular cluster, remarkable, very bright, large, little extended, very much compressed in the middle, partially resolved, some stars seen.

9.0p

–

4.2

7.0

7.1

7.7

9.0

PN

DN

11.6

–

OC/NE 8.0

DNþOC 8.2

DN

DN

OC

OC

GC

OC

OC

14, 21

Cluster ¼ multiple star jh 3780 Flame/Burning Bush Nebula. In same field with Zeta ORI.

4.00 30.00

0.60

27, 30, 32

30.00
20.00 Tarantula Nebula. Surrounds 30 DOR in LMC. Awesome sight!

7, 14

14

14

14

20.00

20.00
15.00 Part of Orion Nebula (M 42). 1,350 LY

14

28.00

Involves 42 ORI, just above Orion Nebula (M 42). 1,350 LY

7

10.00

21

39,500 LY

12.00

27, 30, 32

7, 14

Lies within Large Magellanic Cloud. 179,000 LY

20.00

3.40

18

2158

2169

2232

2239

2244

2251

2261

2264

2286

2301

H VIII-24

H VIII-25

h 392

H VII-2

H VIII-3

H IV-2

H VIII-5 ¼ H V-27

H VIII-31

H VI-27

2129

H VIII-26

H VI-17

NGC/M

Herschel

RA (2000.0)

Dec

06 26.6

04 45

MON 06 51.8 þ00 28 Cluster, rich in stars, large, irregular figure, stars large [bright] and small [faint].

MON 06 47.6 03 10 Cluster, large, compressed, about 100 stars of magnitude 9 to 15.

MON 06 41.1 þ09 53 Extremely large nebula, 3 degrees diameter, densest 120 south preceding 15 MON

MON 06 39.2 þ08 44 Bright, very much extended 330 degrees, nucleus cometic (cometary form) ¼ a star of 11th magnitude.

MON 06 34.7 þ08 22 Cluster, very large, extended, rich in stars, little compressed.

MON 06 32.4 þ04 52 Cluster, beautiful, stars scattered (12 MON).

MON 06 31.0 þ04 57 A star of 8th magnitude in large, poor (sparse) in stars, bright cluster.

MON Bright star (10 MON) plus cluster.

ORI 06 08.4 þ13 57 Cluster, small, little rich in stars, pretty compressed, double star Struve 848 [involved].

GEM 06 07.5 þ24 06 Cluster, pretty small, much compressed, very rich in stars, irregular triangle, stars extremely small [faint].

GEM 06 01.0 þ23 18 Cluster, pretty large, 40 or 50 stars of magnitude 8 to 15.

Con

–

7.3

4.8

4.8

4.2

5.9

8.6

6.7

Mag

OC

OC

6.0

7.5

OCþDN 4.1

DN

OC

OC

DN

OC

OC

OC

OC

Type

14

14

15.00

15.00

8, 14

Christmas Tree Cluster þ Cone Nebula. 2,400 LY

40.00

14

14

Rosette Cluster. Surrounds 12 MON within Nebula. 5,500 LY

24.00

14

Hubble’s Variable Nebula. Surrounds R MON. 2,600 LY

Rosette Nebula. Nebulosity itself not seen by William or John! 5,500 LY

24.00

14

3.00
1.00

Surrounds 10 MON.

45.00

8, 14

14

The “37” Cluster. 3,600 LY

6.00

7, 8

7, 8

Map no.

10.00

In field with open cluster M35 – looks like dim globular. 16,000 LY

Name/Notes

5.00

6.00

Size

19

2354

2353

2360

2359

2362

2371/2372

2392

2422/M 47

2403

2423

H VII-16

H VIII-34

H VII-12

H V-21

H VII-17

H II-316/ H II-317

H IV-45

H VIII-38

H V-44

H VII-28

25 44

PUP 07 37.1 13 52 Cluster, very large, rich in stars, pretty compressed, stars small [faint].

CAM 07 36.9 þ65 36 Remarkable, very much so, considerably bright, extremely large, very much extended, very gradually much brighter to a nucleus.

PUP 07 36.6 14 30 Cluster, bright, very large, pretty rich in stars, stars large [bright] and small [faint].

GEM 07 29.2 þ20 55 Bright, small, round, a [central] star of 9th magnitude, a star of 8th magnitude north following 100 00 .

GEM 07 25.6 þ29 29 Bright, small, round, brighter in the middle to a nucleus, preceding of a double nebula./Pretty bright, small, round, brighter in the middle to a nucleus, following of a double nebula.

CMA 07 18.8 24 57 Cluster, pretty large, rich in stars (30 [Tau] CMA).

CMA 07 18.6 13 12 Remarkable, very much so, very faint, very very large, very irregular figure.

CMA 07 17.8 15 37 Cluster, very large, rich in stars, pretty compressed, stars of magnitude 9 to 12.

MON 07 14.6 10 18 Cluster, large, little compressed, one very bright star.

CMA 07 14.3 Cluster, considerably rich in stars, little compressed.

OC

GX

OC

PN

PN

OC

DN

OC

OC

OC

6.7

8.2

4.4

9.1

11.2

3.8

–

7.2

7.1

6.5

14, 15, 22

14, 15, 22

CH 2 “Caroline’s Cluster” to some, but it’s H VI-30 (below). 6,200 LY Thor’s Helmet/Duck Nebula

Tau Canis Majoris Cluster. 22 Exquisite sight! 5,000 LY Peanut Nebula A bi-polar (double-lobed) planetary.

Clown Face/Eskimo Nebula. 3,000 LY

1,600 LY

18.00

14.00

9.00
6.00

6.00

1.00

0.90

25.00

1, 3, 4

14, 15, 22

23.40
11.80 Often overlooked. 12,000,000 LY

12.00

14, 15, 22

8

6

14, 15, 22

22

18.00

20

2439

2438

2440

2451

2477

2467

2516

2506

2539

H IV-39

H IV-64

h 3099

h 3103

H IV-22

h 3111

H VI-37

H VII-11

2419

H I-218

h 3094

NGC/M

Herschel

RA (2000.0)

Dec

PUP 08 10.7 12 50 Cluster, very large, rich in stars, little compressed, stars of magnitude 11 to 13.

MON 08 00.2 10 47 Cluster, pretty large, very rich in stars, compressed, stars of magnitude 11 to 20.

CAR 07 58.3 60 52 Cluster, very bright, very large, pretty rich in stars, stars of magnitude 7 to 13.

PUP 07 52.6 26 23 Pretty bright, very large, round, easily resolvable, a star of 8th magnitude in the middle.

PUP 07 52.3 38 33 Remarkable, cluster, bright, rich in stars, large, little compressed, a star of 12th magnitude.

PUP 07 45.4 37 58 Cluster, very very large, one star of 4.5 magnitude.

PUP 07 41.9 18 13 Planetary nebula, considerably bright, not very well defined.

PUP 07 41.8 14 44 Planetary nebula, pretty bright, pretty small, very little extended, resolvable (mottled, not resolved), 3.75 seconds diameter.

PUP 07 40.8 31 39 Cluster, bright, pretty rich, pretty large, little compressed, a star of 9th magnitude, stars of magnitude 9 to 14.

LYN 07 38.1 þ38 53 Pretty bright, pretty large, little extended 90 degrees, very gradually brighter in the middle, a star of magnitude 7 or 8 at 267 degrees, 40 distant.

Con

5.8

2.8

9.4

10.8

6.9

10.3

Mag

OC

OC

OC

6.5

7.6

3.8

OCþDN 7.1

OC

OC

PN

PN

OC

GC

Type

3,500 LY

Surrounds 3.6magnitude c PUP. 850 LY At least 300 suns – like loose globular cluster. 4,200 LY 17,000 LY

1,300 LY

1.30

50.00

20.00

15.00

22.00

14, 15

15, 22

12.00

15.00

27, 28, 30

22

22, 27

22, 27

14, 15, 22

14, 15, 22

Projected against open cluster M 46 (at 5,400 LY). 2,900 LY. Very unusual and neat sight!

1.30

3, 8

22

Intergalactic Wanderer. Looks very “remote”! 295,000 LY

4.60

Map no.

9.00

Name/Notes

Size

21

2547

2546

2548/M 48

2808

2792

2818

2867

2841

2910

2903/2905

h 3117

h 3116

H VI-22

h 3152

h 3149

h 3154

h 3163

H I-205

h 3171

H I-56/H I-57

LEO 09 32.2 þ21 30 Considerably bright, very large, extended, gradually much brighter in the middle, resolvable (mottled, not resolved), south preceding of 2./Very faint, resolvable (mottled, not resolved), north following of 2.

VEL 09 30.4 52 54 Cluster, considerably large, pretty rich in stars, pretty compressed, stars of magnitude 10 to 14.

UMA 09 22.0 þ50 58 Very bright, large, very much extended 151 degrees, very suddenly much brighter in the middle ¼ a star of 10th magnitude.

CAR 09 21.4 58 19 Remarkable, very much so, planetary nebula ¼ a star of 8th magnitude, very small, round, a star of 15th magnitude at 59 degrees, 13”.

PYX 09 16.0 36 37 Remarkable, planetary nebula, pretty bright, pretty large, round, very gradually little brighter in the middle, in large cluster.

VEL 09 12.4 42 26 Remarkable, planetary nebula, pretty bright ¼ a star of 9th magnitude, very small, round, among stars.

CAR 09 12.0 64 52 Remarkable, globular cluster, very large, extremely rich in stars, very gradually extremely compressed in the middle, 45 seconds diameter, stars of magnitude 13 to 15.

HYA 08 13.8 05 48 Cluster, very large, pretty rich in stars, pretty much compressed, stars of magnitude 9 to 13.

PUP 08 12.4 37 38 Cluster, bright, large, little compressed, irregularly extended, stars of magnitude 9 to 12.

VEL 08 10.7 49 16 Cluster, bright, large, little compressed, stars of magnitude 7 to 16.

11.6

6.2

5.8

6.3

4.7

GX

OC

GX

PN

8.8

7.2

9.3

9.7

OCþPN 8.2

PN

GC

OC

OC

OC

CH 5. One of formerly “lost” Messier objects. 1,500 LY 31,000 LY

30.00

14.00

8

12.60
6.00

H I-57 is a starcloud in H I-56. Lies all by itself in the sky & easily identified. 20,500,000 LY

27, 28

6.00

3, 4

8.10
3.50

31,000,000 LY

27, 28

22

8.00

0.40

22

27, 28, 30

0.40

Bright planetary in dim cluster. 10,000 LY

22, 27

3,300 LY

70.00

15

22, 27

25.00

22

3034/M 82

3115

3132

3201

3228

3242

3245

3293

3372

H I-163

h 3228

h 3238

h 3245

H IV-27

H I-86

h 3276

h 3295

2997

H V-50

H IV-79

NGC/M

Herschel

RA (2000.0)

Dec

CAR 10 43.8 Remarkable, great nebula, Eta CAR.

CAR 10 35.8 Cluster, bright, rich in stars, pretty large.

59 52

58 14

LMI 10 27.3 þ28 30 Very bright, pretty large, extended 0 degrees, suddenly much brighter in the middle to an extended nucleus.

HYA 10 24.8 18 38 Remarkable, planetary nebula, very bright, little extended 147 degrees, 4500 diameter, blue.

VEL 10 21.8 51 43 Cluster, 9 large [bright] and a few small [faint] stars.

VEL 10 17.6 46 25 Globular cluster, very large, irregularly round, little compressed in the middle, stars of magnitude 13 to 16.

VEL 10 07.0 40 26 Remarkable, very much so, planetary nebula, very bright, very large, little extended, a star of 9th magnitude in the middle, 4 seconds diameter.

SEX 10 05.2 07 43 Very bright, large, very much extended 46 degrees, very gradually then suddenly much brighter in the middle to extended nucleus.

UMA 09 55.8 þ69 41 Very bright, very large, very much extended (ray).

ANT 09 45.6 31 11 Remarkable, very faint, very large, very gradually then very suddenly brighter in the middle to a nucleus 400 , 19.5 seconds in diameter.

Con

DN

OC

GX

PN

OC

GC

PN

GX

GX

GX

Type

3.0p

4.7

10.7

7.7

6.0

6.9

9.2

9.1

8.6

9.4

Mag

Eightburst Planetary/ Southern Ring Nebula. Superb object! 2,000 LY 16,000 LY

1,600 LY

Ghost of Jupiter. Like a big cosmic eye – a beauty! 2,500 LY

1.50

20.00

5.00

1.10

27, 28

Gem Cluster. 8,400 LY Eta Carinae Nebula S. hemisphere spectacle! 10,000 LY

5.00 120.00

27, 28

9

3.20
1.80

15, 16, 23

28

22, 23, 28

22, 23, 28

15, 16

Spindle Galaxy 30,000,000 LY

7.20
2.40

22, 23

1, 3, 4 Bode’s Nebula/Cigar Galaxy Spiral M 81 in same field! 12,000,000 LY

45,000,000 LY

8.90
6.80

Map no.

11.20
4.30

Name/Notes

Size

23

3379/M 105

3521

3556/M 108

3532

3628

3766

3918

3992/M 109

4038

4039

H I-17

H I-13

H V-46

h 3315

H V-8

h 3352

h 3365

H IV-61

H IV-28.1

H IV-28.2

CRV Pretty faint, pretty large.

12 01.9

18 53

CRV 12 01.9 18 52 Pretty bright, considerably large, round, very gradually brighter in the middle.

UMA 11 57.6 þ53 23 Considerably bright, very large, pretty much extended, suddenly brighter in the middle [to a] bright resolvable (mottled, not resolved) nucleus.

CEN 11 50.3 57 11 Planetary nebula, remarkable, small, round, blue, ¼ a star of 7th magnitude, diameter ¼ 1.5 seconds.

CEN 11 36.1 61 37 Cluster, pretty large, pretty rich in stars, pretty compressed, stars of magnitude 8 to 13.

LEO 11 20.3 þ13 36 Pretty bright, very large, very much extended 102 degrees.

CAR 11 06.4 58 40 Remarkable, very much so, cluster, extremely large, round, little compressed, stars of magnitude 8 to 12.

UMA 11 11.5 þ55 40 Considerably bright, very large, very much extended 79 degrees, pretty bright in the middle, resolvable (mottled, not resolved).

LEO 11 05.8 00 02 Considerably bright, considerably large, much extended 140 degrees þ/, very suddenly much brighter in the middle to a nucleus.

LEO 10 47.8 þ12 35 Very bright, considerably large, round, pretty suddenly brighter in the middle, resolvable (mottled, not resolved).

GX

GX

GX

PN

OC

GX

OC

GX

GX

GX

10.4

10.3

9.8

8.1

5.3

9.6

3.0

9.9

9.2

9.5

38,000,000 LY

35,000,000 LY

The Owl Nebula (M 97) lies in same wide field. 45,000,000 LY 1,300 LY

Member of LEO Triplet (together with M 65 and M 66). 35,000,000 LY Pearl Cluster. 5,500 LY Blue Planetary

55,000,000 LY

Antennae/Ringtail Galaxy. Interacting with H IV-28.2 Antennae/Ringtail Galaxy. 90,000,000 LY

5.30
4.80

11.20
5.40

8.60
2.40

50.00

13.10
3.10

15.00

0.40

7.50
4.40

3.40
1.70

3.30
1.70

16, 23

16, 23

4

28

28

9, 16

28

4

16

9, 15, 16

24

4303/M 61

4361

4349

4435

4438

4449

4490

H I-139

H I-65

h 3389

H I-28.1

H I-28.2

H I-213

H I-198

CVN 12 30.6 þ41 38 Very bright, very large, much extended 130 degrees, resolvable (mottled, not resolved), south following of 2.

CVN 12 28.2 þ44 06 Very bright, considerably large, much extended, double or bifurcated, well resolved, clearly consisting of stars, a star of 9th magnitude following 50 .

VIR 12 27.8 þ13 01 Bright, considerably large, very little extended, resolvable (mottled, not resolved), south following of 2.

VIR 12 27.7 þ13 05 Very bright, considerably large, round, north preceding of 2.

CRU 12 24.5 61 54 Cluster, very bright, very large, little compressed, stars of magnitude 12 to 14.

CRV 12 24.5 18 48 Very bright, large, round, very suddenly much brighter in the middle to a nucleus, resolvable (mottled, not resolved).

VIR 12 21.9 þ04 28 Very bright, very large, very suddenly brighter in the middle to a star, binuclear.

CVN 12 19.0 þ47 18 Very bright, very large, very much extended 0 degrees, suddenly brighter in the middle to a bright nucleus.

Dec

4258/M 106

RA (2000.0)

H V-43

Con COM 12 10.1 þ18 33 Globular cluster, very bright, pretty large, round, gradually brighter in the middle, well resolved, clearly consisting of stars.

NGC/M

H I-19 ¼ H I-11 4147 ¼ 4153

Herschel

GX

GX

GX

GX

OC

PN

GX

GX

GC

Type

9.5

9.4

10.0

10.8

7.4

10.9

9.3

8.3

10.4

Mag

The “Eyes”. 40,000,000 LY

13,700,000 LY

Cocoon Galaxy. 4, 9 Faint companion galaxy (H I-197) nearly in contact.

8.50
3.00

6.20
4.40

6.40
3.20

4, 9

9, 16, 31

9, 16, 31

The “Eyes”. 40,000,000 LY

16, 23

3.00
2.20

2,600 LY

2.10

16, 31

28

60,000,000 LY

6.50
5.90

4, 9

9, 16

Map no.

4.00

25,000,000 LY

63,000 LY

4.40

18.60
7.20

Name/Notes

Size

25

COM 12 35.4 þ14 30 Bright, large, little extended, little brighter in the middle.

4548/M 91

4559

4565

4567

4568

4594/M 104

4631

4636

4656

H II-120

H I-92

H V-24

H IV-8

H IV-9

H I-43

H V-42

H II-38

H I-176

CVN 12 44.0 þ32 10 Remarkable, pretty bright, large, very much extended 34 degrees, south preceding of 2.

VIR 12 42.8 þ02 41 Bright, large, irregularly round, very gradually very much brighter in the middle, resolvable (mottled, not resolved).

CVN 12 42.1 þ32 32 Remarkable, very bright, very large, extremely extended 70 degrees þ/, brighter in the middle to a nucleus, a star of 12th magnitude attached north.

VIR 12 40.0 11 37 Remarkable, very bright, very large, extremely extended 92 degrees, very suddenly much brighter in the middle to a nucleus.

VIR 12 36.6 þ11 14 Very faint, large, south following of double nebula.

VIR 12 36.5 þ11 15 Very faint, large, north preceding of double nebula at 160 degrees þ/.

COM 12 36.3 þ25 59 Bright, extremely large, extremely extended 135 degrees, very suddenly brighter in the middle to a nucleus ¼ a star of 10th–11th magnitude.

COM 12 36.0 þ27 58 Very bright, very large, much extended 150 degrees, gradually brighter in the middle, 3 stars following.

VIR 12 34.0 þ07 42 Very bright, very large, much extended 120 degrees þ/, pretty suddenly much brighter in the middle, between 2 stars of 7th magnitude.

H I-38 ¼ H I-31 4526 ¼ H I-119

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

10.1

9.4

9.0

8.3

10.9

11.3

9.5

9.6

10.1

9.6

Siamese Twins. Interacting with H IV-9. 65,000,000 LY Siamese Twins. Interacting with H IV-8. 65,000,000 LY Sombrero Galaxy. Dark “hat brim” and bright nuclear hub – awesome sight! 50,000,000 LY Humpback Whale Galaxy. Tiny galaxy (the “star”) H II-659 just N. 30,000,000 LY

3.10
2.20

4.60
2.20

8.60
4.20

15.20
2.80

16

9

15.30
2.40

9

16, 23

9, 16, 31

5.90
4.60

Hockey Stick Galaxy. 30,000,000 LY

9

Huge edge-on spiral with dark lane along middle! 31,000,000 LY

15.80
2.10

9, 16, 31

9

10.70
4.40

9, 16, 31

5.20
4.20 60,000,000 LY

16, 31

7.00
2.50

26

4697

4725

4755

4945

5005

5053

5128

5139

5195

5248

H I-84

h 3435

h 3459

H I-96

H VI-7

h 3501

h 3504

H I-186

H I-34

4657

H I-177

H I-39

NGC/M

Herschel

RA (2000.0)

Dec

BOO 13 37.5 þ08 53 Bright, large, extended 150 degrees, pretty suddenly brighter in the middle to a resolvable (mottled, not resolved) nucleus.

CVN 13 30.0 þ47 16 Bright, pretty small, little extended, very gradually brighter in the middle, involved in M51.

CEN 13 26.8 47 29 A magnificent or otherwise interesting object, globular cluster, Omega CEN.

CEN 13 25.5 43 01 Remarkable, very much so, very bright, very large, very much extended 122 degrees, bifurcated.

COM 13 16.4 þ17 42 Cluster, very faint, pretty large, irregularly round, very gradually brighter in the middle, stars 15th magnitude.

CVN 13 10.9 þ37 03 Very bright, very large, very much extended 66 degrees, very suddenly brighter in the middle to a nucleus.

CEN 13 05.4 49 28 Bright, very large, very much extended 39 degrees.

CRU 12 53.6 60 20 Cluster, very large, stars very bright (Kappa CRU).

COM 12 50.4 þ25 30 Very bright, very large, extended, very gradually [then] very suddenly very much brighter in the middle to an extremely bright nucleus.

VIR 12 48.6 05 48 Very bright, large, little extended 45 degrees þ/, suddenly much brighter in the middle to a nucleus.

CVN 12 44.2 þ32 12 Remarkable, pretty faint, large, extended 90 degrees þ/, north following of 2.

Con

GX

GX

GC

GX

GC

GX

GX

OC

GX

GX

GX

Type

10.1

9.6

5.3

6.6

9.0

9.8

8.6

4.2

9.3

9.2

12.4

Mag Part of Hockey Stick.

1.30
0.60

23, 28 Omega Centauri Cluster A starry blizzard – superb sight! 16,000 LY Companion to Whirlpool Galaxy (M 51). 37,000,000 LY 50,000,000 LY

55.00

5.90
4.60

6.20
4.50

9, 16, 17

4, 9

23, 24, 28

25.70
20.00 Black Belt Galaxy/CEN A. Big and bright! 15,000,000 LY

9, 16, 17

10.00

Lies just a degree SE of the globular M 53. 53,500 LY

9

5.80
2.90

28, 29

10.00

23, 28

9

10.70
7.60

19.80
4.00

16

9

Map no.

7.20
4.70

Jewel Box/Kappa Crucis Cluster. Radiant and quite beautiful! 7,600 LY

Name/Notes

Size

27

5247

5286

5281

5316

5466

5460

5634

5617

5662

5822

H II-297

h 3533

h 3531

h 3542

H VI-9

h 3555

H I-70

h 3570

h 3573

h 3588

LUP 15 05.2 54 21 Cluster, very large, rich in stars, little compressed, stars of magnitude 9 to 12.

CEN 14 35.2 56 33 Cluster, large, pretty rich in stars, little compressed, stars of 9th magnitude and fainter.

CEN 14 29.8 60 43 Cluster, large, pretty rich in stars, pretty compressed in the middle, stars of 8th magnitude and fainter.

VIR 14 29.6 05 59 Globular cluster, very bright, considerably large, round, gradually brighter in the middle, well resolved, clearly consisting of stars, stars 19th magnitude, a star of 8th magnitude south following.

CEN 14 07.6 48 19 Cluster, very large, very little compressed, stars of 8th magnitude and fainter.

BOO 14 05.5 þ28 32 Cluster, large, very rich in stars, very much compressed, stars of 11th magnitude and fainter.

CEN 13 53.9 62 52 Cluster, pretty large, pretty compressed, stars 11th magnitude.

CEN 13 46.6 62 54 Cluster, bright, small, pretty compressed, irregularly round, stars of magnitude 10 to 12.

CEN 13 46.4 51 22 Globular cluster, very bright, pretty large, round, well resolved, clearly consisting of stars, stars 15th magnitude.

VIR 13 38.1 17 53 Remarkable, very much so, considerably faint, very large, very gradually [then] pretty suddenly much brighter in the middle to a nucleus.

OC

OC

OC

GC

OC

GC

OC

OC

GC

GX

6.5

5.5

6.3

9.5

5.6

9.2

6.0

5.9

7.4

9.9

35.00

28, 29

28, 29

30.00

2,200 LY

28, 29

10.00

17

5.50

82,000 LY

24, 28

35.00

9, 10

52,000 LY

28, 29

9.00

4,200 LY

8.00

28

28, 29

36,000 LY

11.00

16, 17, 23

15.00

50,000,000 LY

5.40
4.90

28

5907

5882

5897

5927

5986

6067

6124

6144

h 3594

H VI-8 ¼ H VI-19

h 3604

h 3611

h 3619

h 3626

H VI-10

5866/M 102

H I-215

H II-759

NGC/M

Herschel

RA (2000.0)

Dec

SCO 16 27.3 26 02 Cluster, considerably large, much compressed, gradually brighter in the middle, well resolved, clearly consisting of stars.

SCO 16 25.6 40 40 Cluster, bright, large, pretty rich in stars, little compressed in the middle, stars of magnitude 9 to 11.

NOR 16 13.2 54 13 Cluster, very bright, very large, very rich in stars, little compressed, stars of 10th magnitude and fainter.

LUP 15 46.1 37 47 Remarkable, globular cluster, very bright, large, round, very gradually brighter in the middle, stars of magnitude 13 to 15.

LUP 15 28.0 50 40 Globular cluster, considerably bright, large, round, very gradually brighter in the middle, well resolved, clearly consisting of stars, stars of 15th magnitude.

LIB 15 17.4 21 01 Globular cluster, pretty faint, large, very irregularly round, very gradually brighter in the middle, well resolved, clearly consisting of stars.

LUP 15 16.8 45 39 Planetary nebula, very small, round, quite sharp.

DRA 15 15.9 þ56 19 Considerably bright, very large, very much extended 155 degrees, very gradually [then] pretty suddenly brighter in the middle to a nucleus.

DRA 15 06.5 þ55 46 Very bright, considerably large, pretty much extended 146 degrees, gradually brighter in the middle.

Con

GC

OC

OC

GC

GC

GC

PN

GX

GX

Type

9.0

5.8

5.6

7.6

8.0

8.4

9.4

10.4

9.9

Mag

25,000 LY

34,000 LY

6.00

9.60

24, 29

18,600 LY

300 NW of Antares and near big globular M 4. 27,700 LY

40.00

7.40

24

29

15.00

24, 29

24, 28, 29

24

40,000 LY

4, 5

11.00

Splinter Galaxy. Ghostly thin needle of light! 40,000,000 LY

12.60
1.40

4, 5

24, 29

Formerly thought to be duplicate of M 101. 40,000,000 LY

6.50
3.10

Map no.

0.30

Name/Notes

Size

29

6171/M 107

6210

6229

6231

6242

6281

6293

6304

6316

6326

H VI-40

h 1970

H IV-50

h 3652

h 3654

h 3664

H VI-12

H I-147

H I-45

h 3675

ARA 17 20.8 51 45 A magnificent or otherwise interesting object, planetary nebula, pretty bright, very small, round.

OPH 17 16.6 28 08 Globular cluster, considerably bright, pretty small, round, gradually very much brighter in the middle, well resolved, clearly consisting of stars, stars 16th magnitude.

OPH 17 14.5 29 28 Globular cluster, bright, considerably large, round, little brighter in the middle, well resolved, clearly consisting of stars, stars 16th magnitude.

OPH 17 10.2 26 35 Globular cluster, very bright, large, round, pretty suddenly brighter in the middle, well resolved, clearly consisting of stars, stars 16th magnitude.

SCO 17 04.8 37 54 Cluster, large, pretty rich in stars, little compressed, stars of magnitude 9 to 11.

SCO 16 55.6 39 30 Cluster, bright, large, rich in stars, stars of magnitude 8 to 11.

SCO 16 54.0 41 48 Cluster, bright, considerably large, pretty rich in stars, stars of magnitude 10 to 13.

HER 16 47.0 þ47 32 Globular cluster, very bright, large, round, disc & faint border, resolvable (mottled, not resolved).

HER 16 44.5 þ23 49 Planetary nebula, very bright, very small, round, disc & border, (nucleus variable?).

OPH 16 32.5 13 03 Globular cluster, large, very rich in stars, very much compressed, round, well resolved, clearly consisting of stars.

PN

GC

GC

GC

OC

OC

OC

GC

PN

GC

Originally thought to be a planetary nebula. 99,000 LY

Table of Scorpius Cluster. 24, 29 6,000 LY 4,000 LY

4.50

14.00

9.00

24

28,700 LY

19,600 LY

Tiny, but bright and rich. 36,000 LY

8.20

8.00

5.40

29

24

24

24

8.00

24, 29

5, 10

10

¼ Struve 5N. Cobalt-blue little gem. 3,600 LY

0.40

17, 18, 24

21,000 LY

13.00

12.2p 0.30

8.1

8.3

8.3

5.4

6.4

2.6

9.4

8.8

7.8

30

6369

6362

6388

6397

6445

6441

6543

6514/M 20

h 3684

h 3690

h 3692

H II-586

h 3705

H IV-37

H IV-41, H V10, 11 and 12

6356

H I-48

H IV-11

NGC/M

Herschel

RA (2000.0)

Dec

SGR 18 02.3 23 02 A magnificent or otherwise interesting object, very bright, very large, trifid, double star involved.

DRA 17 58.6 þ66 38 Planetary nebula, very bright, pretty small, suddenly brighter in the middle [to a] very small nucleus.

SCO 17 50.2 37 03 Globular cluster, very bright, pretty large, round, very gradually much brighter in the middle, well resolved, clearly consisting of stars, stars 18th magnitude.

SGR 17 49.2 20 01 Pretty bright, pretty small, round, gradually brighter in the middle, resolvable (mottled, not resolved), star of 15th magnitude north preceding.

ARA 17 40.7 53 40 Globular cluster, bright, very large, rich in stars, stars 13th magnitude.

SCO 17 36.3 44 44 Globular cluster, very bright, large, round, pretty gradually [then] pretty suddenly very much brighter in the middle, well resolved, clearly consisting of stars, stars 17th magnitude and fainter.

ARA 17 31.9 67 03 Globular cluster, considerably bright, large, very gradually much brighter in the middle, well resolved, clearly consisting of stars, stars of magnitude 14 to 17.

OPH 17 29.3 23 46 Remarkable, very much so, ring, pretty bright, small, round.

OPH 17 23.6 17 49 Globular cluster, very bright, considerably large, very gradually very much brighter in the middle, well resolved, clearly consisting of stars, stars 20th magnitude.

Con

DN

PN

GC

PN

GC

GC

GC

PN

GC

Type

6.3

8.1

7.2

11.2

5.3

6.8

8.1

11.4

8.2

Mag

32,600 LY

7,200 LY

Little Gem Nebula. Also known as Crescent Nebula (along with H IV72 in CYG below).

3rd magnitude G SCO lies 24, 25 very close-by in field. 38,000 LY

Cat0 s Eye/Snail Nebula. Famous! 3,600 LY Various sections of the Trifid Nebula. 5,200 LY

10.40

31.00

0.70

9.60

0.30

20.00

24, 25

1, 5

18, 24

29

24, 25, 29

29, 30

24,800 LY

15.00

24

18, 24

Map no.

Little Ghost Nebula. Haunting sight! 3,800 LY

Name/Notes

0.60

10.00

Size

31

6523/M 8

6530

6541

6572

6633

6712

6723

6752

6819

6818

H V-9 & H V-13

h 3725

h 3726

h 2000

H VIII-72

H I-47

h 3770

h 3778

h 2048

H IV-51

SGR 19 44.0 14 09 Planetary nebula, bright, very small, round.

CYG 19 41.3 þ40 11 Cluster, very large, very rich in stars, stars of magnitude 11 to 15.

PAV 19 10.9 59 59 Globular cluster, bright, very large, irregularly round, well resolved, clearly consisting of stars, stars of magnitude 11 to 16.

SGR 18 59.6 36 38 Globular cluster, very large, very little extended, very gradually brighter in the middle, well resolved, clearly consisting of stars, stars of magnitude 14 to 16.

SCT 18 53.1 08 42 Globular cluster, pretty bright, very large, irregular, very gradually little brighter in the middle, well resolved, clearly consisting of stars.

OPH 18 27.7 þ06 34 Cluster, little compressed, stars large [bright].

OPH 18 12.1 þ06 51 Planetary nebula, very bright, very small, round, little hazy.

CRA 18 08.0 43 42 Globular cluster, bright, round, extremely compressed, gradually brighter in the middle, well resolved, clearly consisting of stars, stars of magnitude 15 to 16.

SGR 18 04.8 24 20 Cluster, bright, large, pretty rich in stars, following M8.

SGR 18 03.8 24 23 A magnificent or otherwise interesting object, very bright, extremely large, extremely irregular figure, with large cluster.

PN

OC

GC

GC

GC

OC

PN

GC

OC

DN

9.3

7.3

5.3

6.8

8.1

4.6

8.1

6.3

4.6

5.0p

Various sections of the Lagoon Nebula. 5,200 LY

Involved with Lagoon Nebula. 23,000 LY

¼ Struve 6N Blue-green tiny gem. 1,900 LY CH 8. 1,000 LY 22,500 LY

28,400 LY

Pavo Globular Cluster. A beauty! 13,000 LY

Foxhead Cluster, CH 16. 7,200 LY Little Gem Nebula. Turquoise-blue dot. 5,000 LY

45.00

15.00

15.00

0.20

20.00 9.80

13.00

29.00

5.00

0.80

18, 19, 25

5, 11

26, 29, 30

25

18

18

18

24, 25, 29

24, 25

24, 25

32

6866

6888

6905

6939

6940

6946

6960

6992

6995

H IV-72

H IV-16

H VI-42

H VII-8

H IV-76

H V-15

H V-14

h 2093

6826

H IV-73

H VII-59

NGC/M

Herschel

RA (2000.0)

Dec

CYG 20 57.1 þ31 13 Faint, extremely large, nebula & stars in groups.

CYG 20 56.4 þ31 43 Remarkable, very much so, extremely faint, extremely large, extremely extended, extremely irregular figure, bifurcated.

CYG 20 45.7 þ30 43 Remarkable, very much so, pretty bright, considerably large, extremely irregular figure, 52 CYG involved.

CEP 20 34.8 þ60 09 Very faint, very large, very gradually [then] very suddenly brighter in the middle, partially resolved, some stars seen.

VUL 20 34.6 þ28 18 Cluster, very bright, very large, very rich in stars, considerably compressed, stars pretty large [bright].

CEP 20 31.4 þ60 38 Cluster, pretty large, extremely rich in stars, pretty compressed in the middle, stars of magnitude 11 to 16.

DEL 20 22.4 þ20 07 Remarkable, very much so, planetary nebula, bright, pretty small, round, 4 small [faint] stars near.

CYG 20 12.0 þ38 21 Faint, very large, very much extended, two stars attached.

CYG 20 03.7 þ44 00 Cluster, large, very rich in stars, considerably compressed.

CYG 19 44.8 þ50 31 Planetary nebula, bright, pretty large, round, a star of 11th magnitude in the middle.

Con

SR

SR

SR

GX

OC

OC

PN

DN

OC

PN

Type

Name/Notes Blinking Planetary. Alternate between direct and averted vision to see! 3,300 LY Kite Cluster, CH 7. 4,000 LY

Size 0.60

7.00

7.0

7.0

7.0

9.0

6.3

7.8

11.1

Blue Flash Nebula. 4,200 LY In same field with H IV-76 (below). 4,000 LY

2,500 LY

In same field with H VI-42 (above). 10,000,000 LY

Veil/Filamentary/Cirrus Nebula. Vast supernova bubble. 2,600 LY Veil/Filamentary/Cirrus Nebula. Section of bubble or “Loop.” Veil/Filamentary/Cirrus Nebula. Section of bubble or “Loop.”

1.20

10.00

25.00

11.50
9.80

70.00
0.60

60.00
8.00

12.00

10.0p 18.00
13.00 Crescent Nebula

7.6

8.8

Mag

11

11

11

1, 2, 5

11

1, 2, 5

11, 19

5, 11

5, 11

5, 11

Map no.

33

7000

7023

7009

7243

7331

7380

7635

7662

7789

H V-37

H IV-74

H IV-1

H VIII-75

H I-53

H VIII-77

H IV-52

H IV-18

H VI-30

CAS 23 57.0 þ56 44 Cluster, very large, very rich in stars, very much compressed, stars of magnitude 11 to 18.

AND 23 25.9 þ42 33 A magnificent or otherwise interesting object, planetary nebula or ring, very bright, pretty small, round, blue, variable nucleus.

CAS 23 20.7 þ61 12 Very faint, a star of 8th magnitude involved, little eccentric.

CEP 22 47.0 þ58 06 Cluster, pretty large, pretty rich in stars, little compressed, stars of magnitude 9 to 13.

PEG 22 37.1 þ34 25 Bright, pretty large, pretty much extended 163 degrees, suddenly much brighter in the middle.

LAC 22 15.3 þ49 53 Cluster, large, poor (sparse) in stars [??], little compressed, stars very large [bright].

AQR 21 04.2 11 22 A magnificent or otherwise interesting object, planetary nebula, very bright, small, elliptic.

CEP 21 00.5 þ68 10 A star of 7th magnitude in extremely faint [??], extremely large nebulosity.

CYG 20 58.8 þ44 20 Faint, extremely large, diffused nebulosity.

4.0p

9.5

6.4

8.0

OC

PN

DN

Iris Nebula. Nebulosity is actually bright and easy!? Saturn Nebula ¼ Struve 8N. An amazing and eerie sight! 2,400 LY Dim triple Struve 2890 in center. 2,800 LY One of brighter nonMessier galaxies. 46,000,000 LY CH 19. 7,200 LY

10.00
8.00

0.60

30.00

10.20
4.20

20.00

6.7

8.3

25.00

0.60

2

2

6

2

19, 25

1, 2, 5

5, 11

Caroline’s Cluster, CH 14. 300þsuns. Stardust – beautiful sight! 7,600 LY

2

Blue Snowball. Bluish and 2, 6 bright! 5,600 LY

Bubble Nebula. In wide field with open cluster M 52.

North America Nebula Huge! 1,600 LY

120.00
100.00

11.0p 15.00
8.00

OCþDN 7.2

GX

OC

PN

DNþOC 7.1p

DN

34

The Cambridge Atlas of Herschel Objects

Some recommended references Of the extensive literature existing on the subject of the Herschels and their discoveries, the following are a number of the most useful and interesting print and electronic publications. Although some of the older classic works have been reprinted, others are now out of print but still to be found in used book stores, observatory libraries, and also over the Internet. And while the numerical/physical parameters they give for these objects is in most cases quite dated, their descriptive accounts have a charm, passion, and warmth about them that’s sadly missing from many such guides today. B. Branchett, Observe: The Herschel Objects, The Astronomical League, East Peoria, IL, 1980. The original manual for observing the 400 Herschel objects selected as targets for the US-based Astronomical League’s Herschel 400 Club. (See below for its sequel which contains an additional 400 objects.) For more information, go to: http://astroleague.org/al/obsclubs/ herschel/hers400.html M. Bratton, The Complete Guide to the Herschel Objects, Cambridge University Press, Cambridge, publication due 2011. This major new observing reference provides a complete re-examination of William Herschel’s entire catalogue of some 2,500 star clusters and nebulae (many of the latter being galaxies, unrecognized as such in his time), while retracing the footsteps of this great astronomer’s life as an observer and telescope maker. Contains detailed notes about each object’s visual appearance (including those considered lost or nonexistent), and includes hundreds of images of the most fascinating wonders supplemented by dozens of eyepiece sketches. This amazing book is destined to become the ultimate reference on Sir William’s pioneering discoveries. R. Burnham, Jr., Burnham’s Celestial Handbook, Volumes 1, 2 and 3, Dover Publications, New York, 1978. One of the most comprehensive guidebooks to the heavens ever written, this modern classic covers some 7,000 celestial wonders including many Herschel objects. Simply a “must have”! A. Clerke, The Herschels and Modern Astronomy, Cassell and Company, London, 1895. A charming overview of all three Herschels and their impact on astronomy of the time. C. Cole and C. Pratt, Observe: The Herschel II Objects, The Astronomical League, West Burlington, IA, 1997. A follow-up manual to the original roster (see above), giving 400 more Herschel objects selected as targets for the US-based Astronomical League’s Herschel Club.

J. L. E. Dreyer, New General Catalogue of Nebulae and Clusters of Stars, Royal Astronomical Society, London, 1971. The ultimate reference covering all of the discoveries of both William and John Herschel (including those objects actually found by Caroline Herschel). J. L. E. Dreyer (ed.), Scientific Papers of Sir William Herschel, The Royal Society, London, 1912. This compendium, reprinted jointly by the Royal Society and the Royal Astronomical Society, is an extremely valuable reference for those desiring to read William Herschel’s published papers without having access to the Philosophical Transactions in which they originally appeared. D. Evans, Herschel at the Cape, University of Texas at Austin, Austin, TX, 1969. A work devoted exclusively to the many discoveries of Sir John Herschel during his famous survey of the southern sky at Cape Town, South Africa. H. Frommert, The Interactive NGC Catalog Online. A superb Internet resource for the latest updated version of the original NGC and its two Index Catalogues. Also contains images of each object from the Digital Sky Survey. To access it go to www.seds.org/~spider/ngc/ ngc.html or simply enter its title in your computer’s search window. E. Hartung, Astronomical Objects for Southern Telescopes, Cambridge University Press, Cambridge, 1998. Perhaps the ultimate descriptive work on the visual appearance of deep-sky wonders of all types as seen from the Southern Hemisphere. (Also includes many objects visible from the Northern Hemisphere.) A. Hirshfield and R. Sinnott, Sky Catalogue 2000.0, Volume 2, Sky Publishing and Cambridge University Press, Cambridge, 1985. A companion volume to Wil Tirion’s famed Sky Atlas 2000.0, it contains data on thousands of deep-sky wonders plotted in the Atlas itself including many Herschel objects (listed by their NGC numbers only). E. S. Holden, Sir William Herschel, Charles Scribner’s Sons, New York, 1881. An excellent in-depth account of William’s life and work one of the very finest ever written. M. Hoskin, The Herschel Partnership: As Viewed by Caroline, Science History Publications Ltd., London, 2003. Offers fascinating new insights into the working relationship between Sir William and his devoted sister by a noted historian of astronomy. M. Hoskin, William Herschel and the Construction of the Heavens, Norton and Norton, New York, 1964. Yet another, earlier contribution by Hoskin, focusing on Sir William’s cosmology.

Some recommended references

35

H. C. King, The History of the Telescope, Dover Publications, New York, 2003. Has one of the best concise accounts to be found of William Herschel’s life, telescopes, and work.

of Arizona Press, Tucson, AZ, 1973. The comprehensive update of the original NGC containing the notorious “nonexistent” Herschel objects based on the Palomar Sky Survey photographic plates.

C. Lubbock, The Herschel Chronicle: The Life Story of William Herschel and His Sister Caroline Herschel, Cambridge University Press, Cambridge, 1933; reprinted by the William Herschel Society, London, in 1997. One of the most in-depth accounts of these two Herschels ever published.

W. Steinicke, Revised NGC and IC Catalog. This superb Internet resource offers the very latest data available online for the original NGC and its two Index Catalogues. To access it, go to the site for The Interactive NGC Catalog Online (see above) and click on the Revised NGC/IC data link shown.

J. Mullaney, The Herschel Objects and How to Observe Them, Springer-Verlag, New York, 2007. An upbeat, non-technical overview of the subject by the co-author of this Atlas emphasizing the pleasure to be derived from observation of these objects. Features images and descriptions of 165 of the best showpieces from Sir William’s catalog.

W. Steinicke, Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer’s New General Catalogue, Cambridge University Press, Cambridge, 2010. The fascinating history of the discovery, observation, description and cataloguing of star clusters and nebulae in the nineteenth century has largely gone untold until now! This well-researched volume is the first comprehensive historical study of the NGC itself, and is an important resource for those interested in the history of astronomy in general and visual deep-sky observing in particular. It covers the people, observatories, telescopes and techniques used during this golden age of discovery, as well as many prominent deep-sky wonders themselves.

J. Mullaney, Celestial Harvest: 300-Plus Showpieces of the Heavens for Telescope Viewing & Contemplation, Dover Publications, New York, 2002. This work, originally self-published in 1998, contains extensive descriptions of many of the finest Herschel objects by both classic and modern-day observers. S. J. O’Meara, Steve O’Meara’s Herschel 400 Observing Guide, Cambridge University Press, Cambridge, 2007. Comprehensive coverage of the Herschel Club’s original target list of 400 objects written by the foremost visual observer in the world today. Features detailed finder charts, vivid descriptions, and eyepiece sketches of each entry. J. B. Sidgwick, William Herschel, Explorer of the Heavens, Faber and Faber, London, 1953. Comprehensive work by a noted British authority on observational astronomy. R. W. Sinnott (ed.), NGC 2000.0, Sky Publishing Corporation and Cambridge University Press, Cambridge, MA, and London, 1988. An updated and corrected version of Dreyer’s original NGC and its two Index Catalogues for the current standard positional Epoch 2000.0. W. H. Smyth, The Bedford Catalogue, being Volume Two of A Cycle of Celestial Objects, Willmann-Bell, Inc., Richmond, VA, 1986. This reprinted classic from 1844 is the one that really “started it all” in terms of turning observers on to the fascinating world of deep-sky observing with small instruments. It contains detailed and often very quaint descriptions of the visual appearance of many of the brighter Herschel objects using Sir William’s original designations. J. Sulentic and W. Tifft, The Revised New General Catalogue of Nonstellar Astronomical Objects, University

T. W. Webb, Celestial Objects for Common Telescopes, Cambridge University Press, Cambridge, 2010. First published in 1859 as a single volume, this charming classic quickly became the most beloved and used guidebook of its day, and its popularity has continued right up to the present time despite being out-of-print. In later editions, it was split into two volumes containing nearly 4,000 targets (the majority being double and multiple stars). With the exception of the Messier objects, the clusters and nebulae described in it were given with their original Herschel (as well as NGC) designations. This classic is once more available as a self-contained single volume in this new edition from Cambridge.

Some additional valuable resources are the various publications of The William Herschel Society of Bath, UK (www.williamherschel.org.uk), and the Webb Deep Sky Society of London, UK (www. webbdeepsky.com). Also, the two US based magazines Astronomy (www.astronomy.com) and, especially, Sky & Telescope (www.skyandtelescope. com) have run many articles about the Herschels (including ones by the author) over the years. Finally, the Journal for the History of Astronomy (www.shpltd. co.uk/jha.html) is an excellent scholarly work often containing papers about the Herschels.

36

The Cambridge Atlas of Herschel Objects

About the authors Wil Tirion had no formal education in astronomy. His training was focused on graphic art and design, although the starry sky and especially star maps have always fascinated him. In the fields of astronomy and uranography (mapping the sky), he is what is known as an “autodidact.” In 1977, purely for his own enjoyment, he started making his first star atlas, which showed stars down to magnitude 6.5. It was published in the Encyclopedia of Astronomy, edited by Colin Ronan (Hamlyn, London, 1979) and in 1981 as a separate set of maps by the British Astronomical Association (BAA Star Charts 1950.0). In 1978, still as a hobby, he started working on a larger atlas entitled Sky Atlas 2000.0, showing stars down to magnitude 8.0. Its publication in 1981 (Sky Publishing Corporation, USA, co-published by Cambridge University Press, UK), resulted in requests from several additional publishers to execute star maps for a variety of purposes. In 1983 he decided to quit his job as a graphic artist and designer, and become a full-time uranographer. Since then he has created such popular star atlases as the Bright Star Atlas 2000.0 and the The Cambridge Star Atlas, and has cooperated with others on much larger atlases like Uranometria 2000.0. He has also created numerous star maps for various astronomy books and magazines. In 1987 he was honored by receiving the “Dr. J. van der Bilt Prize,” a Dutch award for outstanding work by amateur astronomers. This was followed in 1993 by a more international “award” when minor planet 4648 Tirion (1931 UE) was named after him. His website is: www.wil-tirion.com. James Mullaney is an astronomy writer, lecturer and consultant who has published more than 500 articles and seven books (including The Cambridge Double Star Atlas) on observing the wonders of the heavens, and logged over 20,000 hours of stargazing time with the unaided eye, binoculars and telescopes. Formerly Curator of the Buhl Planetarium & Institute of Popular Science in Pittsburgh and Director of the DuPont Planetarium, he served as staff astronomer at the University of Pittsburgh’s Allegheny Observatory and as an assistant editor for

Sky & Telescope magazine. He was also one of the contributors to Carl Sagan’s award-winning Cosmos PBS-Television series. His 50-year mission has been to “Celebrate the Universe!” to get others to look up at the majesty of the night sky and to personally experience the joys of stargazing. In February of 2005 he was elected a Fellow of the prestigious Royal Astronomical Society of London.

Acknowledgements It has been a sincere pleasure working on this project from its very inception with Vince Higgs, Commissioning Editor, Astronomy and Astrophysics, at Cambridge University Press. It was he who had the vision to see the need for this seminal new star atlas as proposed by author Mullaney, and he who obtained the endorsement of the Cambridge University Press editorial review board and management to undertake its publication. Special acknowledgement is also due Hartmut Frommert and Wolfgang Steinicke for creating/maintaining their immensely valuable The Interactive NGC Catalog Online and Revised NGC and IC Catalog, respectively. And thanks to Dr. Michael Hoskin, founder and editor of The Journal for the History of Astronomy, for valuable information about the Herschels, especially Caroline and her discoveries. Lindsay Barnes, Laura Clark, Claire Poole, and Jonathan Ratcliffe at Cambridge all played roles in bringing this Atlas to press. Wil Tirion wants to thank James ( Jim) Mullaney for his valuable input in this project. Without his expertise on the subject, and his great practical experience in observing the Herschel objects, it would not have been possible to create this Atlas. For James Mullaney, it has been a great honor and rare privilege to again work closely with the famed and immensely talented Wil Tirion, creator of many legendary previous star atlases and who is without question the greatest mapper of the starry heavens the world has ever known. This collaboration has resulted in a truly unique new work in the field of astronomy that is sure to be actively used and endorsed by “Herschelians” worldwide.

STAR CHARTS

HYI

Appendix A:

Constellation table

The following list gives the full names of the 88 officially recognized constellations, together with their genitive (possessive) cases, order of size in terms

of number of square degrees, standard International Astronomical Union (IAU) three letter abbreviations, and Atlas map number/s on which they are shown.

Name

Genitive

Size

Abbrev.

Map number/s

Andromeda

Andromedae

19

AND

6

2

7

Antlia

Antliae

62

ANT

23

22

28

Apus

Apodis

67

APS

30

29

28

Aquarius

Aquarii

10

AQR

19

12

20

Aquila

Aquilae

22

AQL

19

18

11

25

Ara

Arae

63

ARA

29

30

28

Aries

Arietis

39

ARI

7

6

13

Auriga

Aurigae

21

AUR

3

7

8

Boo¨tes

Boo¨tis

13

BOO

10

9

17

16

2

4

Caelum

Caeli

81

CAE

21

27

Camelopardalis

Camelopardalis

18

CAM

1

3

Cancer

Cancri

31

CNC

8

15

Canes Venatici

Canum Venaticorum

38

CVN

9

4

10 15

Canis Major

Canis Majoris

43

CMA

22

14

Canis Minor

Canis Minoris

71

CMI

15

14

Capricornus

Capricorni

40

CAP

19

25

Carina

Carinae

34

CAR

27

28

Cassiopeia

Cassiopeiae

25

CAS

2

3

1

Centaurus

Centauri

9

CEN

28

23

24

Cepheus

Cephei

Cetus

Ceti

Chamaeleon

Chamaeleontis

30

27

CEP

2

1

5

4

CET

13

12

20

79

CHA

30

28

27

Circinus

Circini

85

CIR

28

29

30

Columba

Columbae

54

COL

21

22

27

Coma Berenices

Comae Berenices

42

COM

9

16

17

Corona Australis

Coronae Australis

80

CRA

25

24

29

Corona Borealis

Coronae Borealis

73

CRB

10

5

Corvus

Corvi

70

CRV

23

16 16

Crater

Crateris

53

CRT

23

Crux

Crucis

88

CRU

28

Cygnus

Cygni

16

CYG

11

5

Delphinus

Delphini

69

DEL

19

11

Dorado

Doradus

7

DOR

27

30

Draco

Draconis

8

DRA

5

4

Equuleus

Equulei

87

EQU

19

11

12

2

29 21

6

1

103

4

5

104

The Cambridge Atlas of Herschel Objects

Name

Genitive

Size

Abbrev.

Map number/s

Eridanus

Eridani

Fornax

Fornacis

6

ERI

21

13

14

41

FOR

21

20

26

Gemini

Geminorum

30

Grus

Gruis

45

GEM

8

14

15

GRU

20

26

25

Hercules

Herculis

5

HER

10

11

5

Horologium

Horologii

58

HOR

27

26

21

Hydra

Hydrae

1

HYA

15

23

22

Hydrus

Hydri

61

HYI

26

30

27

Indus

Indi

49

IND

26

29

30

Lacerta

Lacertae

68

LAC

2

6

11

Leo

Leonis

12

LEO

9

16

15

Leo Minor

Leonis Minoris

64

LMI

9

8

4

Lepus

Leporis

51

LEP

21

14

22

Libra

Librae

29

LIB

24

17

26

27

18

17

24

26

8

Lupus

Lupi

46

LUP

24

29

28

Lynx

Lyncis

28

LYN

3

8

4

Lyra

Lyrae

52

LYR

11

5

Mensa

Mensae

75

MEN

30

27

Microscopium

Microscopii

66

MIC

25

Monoceros

Monocerotis

35

MON

14

15

Musca

Muscae

77

MUS

28

30

Norma

Normae

74

NOR

29

28

24

Octans

Octantis

50

OCT

30

26

29

Ophiuchus

Ophiuchi

11

OPH

18

24

17

10

Orion

Orionis

26

ORI

14

7

8

13

Pavo

Pavonis

44

PAV

30

29

26

Pegasus

Pegasi

7

PEG

6

19

12

Perseus

Persei

24

PER

7

3

2

Phoenix

Phoenicis

37

PHE

26

20

21

Pictor

Pictoris

59

PIC

27

30

Pisces

Piscium

14

PSC

12

6

Piscis Austrinus

Piscis Austrini

60

PSA

20

25

Puppis

Puppis

20

PUP

22

27

15

26

30

Pyxis

Pyxidis

65

PYX

22

Reticulum

Reticuli

82

RET

27

8

11

13 14

Sagitta

Sagittae

86

SGE

11

19

18

Sagittarius

Sagittarii

15

SGR

25

24

18

19

29

Scorpius

Scorpii

33

SCO

24

17

18

25

29

Sculptor

Sculptoris

36

SCL

20 10

24

Scutum

Scuti

84

SCT

18

25

Serpens

Serpentis

23

SER

17

18

Sextans

Sextantis

47

SEX

15

16

Taurus

Tauri

17

TAU

7

13

Telescopium

Telescopii

57

TEL

29

25

14

Appendix A: Constellation table

Name

Genitive

Size

Abbrev.

105

Map number/s

Triangulum

Trianguli

78

TRI

7

6

2

Triangulum Australe

Trianguli Australis

83

TRA

30

29

28

Tucana

Tucanae

48

TUC

26

29

30

Ursa Major

Ursae Majoris

3

UMA

4

9

3

Ursa Minor

Ursae Minoris

56

UMI

1

4

5

Vela

Velorum

32

VEL

28

27

22

23

Virgo

Virginis

2

VIR

16

17

23

9

Volans

Volantis

76

VOL

30

27

28

Vulpecula

Vulpeculae

55

VUL

11

5

1

24

Appendix B: The Cambridge Atlas of Herschel Objects target list 2,500þ Clusters, nebulae, and galaxies arranged by right ascension Key/Notes: OC open cluster GC globular cluster PN planetary nebula DN diffuse nebula SR supernova remnant GX galaxy NE “nonexistent” H William Herschel CH Caroline Herschel h John Herschel NGC New General Catalogue M Messier SMC Small Magellanic Cloud LMC Large Magellanic Cloud MW Milky Way * Herschel Club 400 List The nominal visual magnitude limit is 12.5. A number of fainter objects are included for the reasons given in the text. The letter “p” indicates a photographic magnitude rather than a visual one,

106

which averages roughly a magnitude brighter than what the eye sees if the object is blue in hue and a magnitude fainter if it’s yellow or red. An explanation of the column headers will be found in the Herschel showpiece section of the text. Note that under the map column some numbers are in italics, meaning that the object is plotted on that map but is unlabeled: this only occurs in areas that are covered in more detail by the two extra maps, 31 and 32. The primary print and online data sources used in compiling the following roster were:  New General Catalogue of Nebulae and Clusters of Stars by J. L. E. Dreyer  NGC 2000.0 by Roger W. Sinnott  The Interactive NGC Catalog Online by Hartmut Frommert  Revised NGC and IC Catalog by Wolfgang Steinicke  The Revised New General Catalogue of Nonstellar Astronomical Objects by J. W. Sulentic and W. G. Tiff  SIMBAD Astronomical Database

107

125 128 129

H III-869

H II-854

H VIII-79 *

147 151 148

h 29

H II-478

h 2329

146

121

h 2325

152

110

h 22

h 28

108

H III-148

h 2331

SCL

103

h 20

134

104

h 2322

136

97

h 18

h 2327

95

H II-257

H VI-35 *

CAS

80

h 16

SCL

SCL

CET

CAS

CAS

TUC

CAS

PSC

PSC

TUC

CAS

AND

CAS

TUC

AND

PSC

AND

PSC

55

CET

57

45

h 2313

CEP

H II-241 ¼ II-243

40

H IV-58 *

SCL

PEG

PEG

PEG

SCL

CET

PEG

CEP

PEG

CAS

Con

h 2315

23

16

H IV-15 24

14

H II-591

H III-147

10

h 4015

H III-461

7817

7822

h 2302 7826

7814

H II-240

H VIII-29

7801

h 2292

H II-227

NGC/M

Herschel

00 34.3

00 34.0

00 33.2

00 33.1

00 32.8

00 31.5

00 30.4

00 29.9

00 29.2

00 28.8

00 26.8

00 27.4

00 25.9

00 25.3

00 24.1

00 22.4

00 22.2

00 21.2

00 15.4

00 14.9

00 14.1

00 13.0

00 09.9

00 09.9

00 09.1

00 08.8

00 08.6

00 05.2

00 04.0

00 03.6

00 03.3

00 00.4

31 47

09 42

þ48 30

þ63 18

73 09

þ61 32

33 15

þ60 14

þ02 51

þ02 50

71 32

þ71 23

þ29 13

þ61 21

72 05

þ29 44

þ10 30

þ22 21

þ17 18

39 11

23 11

þ72 32

24 58

þ25 55

þ27 44

þ15 49

33 52

20 44

þ20 45

þ68 37

þ16 09

þ50 42

RA (2000.0) Dec

GX

GX

GX

OC

OC

OC

GX

OC

GX

GX

GC

OC

GX

OC

GC

GX

GX

GX

GX

GX

GX

PN

GX

GX

GX

GX

GX

OC/NE

GX

DN

GX

OC/NE

Type

12.1

12.4

9.4

9.1

11.9p

–

10.4

6.5

11.8

12.4

11.2

–

12.2

9.8

4.0

12.4

12.5

12.2

11.8

7.8

10.7

12.3?

11.5

11.9

12.0

12.2

12.3

–

11.8

–

10.8

–

Mag

0

0

0

h5

0

21.00

0

2.00  0.80

3.80  1.60

13.2  7.8

5.00

1.7

0

1.50

8.4  1.8

h 30 ¼ h 2330

in SMC

h 24

2.50  0.70 0

h 25

1.80  1.60

0

h 23

1.50

20

12

2, 6

2

26, 30

2

20

2

12

12

1, 2 26, 30

in SMC

19.00

2 6

2.30  1.80

h 21

5.00

6 26, 30

31.00

47 Tucanae Cluster

1.30

6 12

h 19

1.50  1.10

6, 12

1.60

h 13

20

2.20  1.90

31.2  5.9

20

1, 2

0

h 8, magnitude highly uncertain (10.2?)

1.20

20

6

6

6, 12

20

20

6

2

6, 12

2, 6

Map no.

8.50  5.90

h 2308

5.80  1.30

2.1  1.3

0

0

h3

2.8  2.1 1.80  1.00

h 2305

h 2300

likely SR

h 2297

Name/Notes

0

0

2.40  1.20

12.00

3.5  1.0

0

100.00

5.5  2.3

0

15.0

0

Size

108

NGC/M 157 173 175 ¼ 171 182 185 193 194 189 205/M 110

220 206 210 222 214 227 221/M32 224/M 31 225 245 246 247 188 254 253 265 255 252 266

Herschel

H II-3 *

H III-871

H III-223

H III-870

H II-707 *

H III-595

H II-856

h 36

H V-18 *

h 2338

H V-36

H II-452

h 2339

H II-209

H II-444

h 51

h 50

H VIII-78 *

H II-445

H V-25 *

H V-20 *

h 34

h 2347

H V-1 *

h 2351

H II-472

H II-609

H III-153

PSC

AND

CET

TUC

SCL

SCL

CEP

CET

CET

CET

CAS

AND

AND

CET

AND

TUC

CET

AND

TUC

AND

CAS

PSC

PSC

CAS

PSC

CET

CET

CET

Con

00 49.8

00 48.0

00 47.8

00 47.6

00 47.6

00 47.5

00 47.5

00 47.1

00.47.0

00 46.1

00 43.4

00 42.7

00 42.7

00 42.6

00 41.5

00 40.6

00 40.6

00 40.6

00 40.5

00 40.4

00 39.6

00 39.3

00 39.3

00 39.0

00 38.2

00 37.4

00 37.2

00 34.8

þ32 16

þ27 38

11 28

73 29

25 17

31 25

þ85 20

20 46

11 53

01 44

þ61 47

þ41 16

þ40 52

01 32

þ25 30

73 24

13 52

þ40 44

73 24

þ41 41

þ61 04

þ03 02

þ03 20

þ48 20

þ02 44

19 56

þ01 56

08 24

RA (2000.0) Dec

GX

GX

GX

GC

GX

GX

OC

GX

PN

GX

OC

GX

GX

GX

GX

OC

GX

OC

OC

GX

OC

GX

GX

GX

GX

GX

GX

GX

Type

11.8

12.5

11.9

12.2

7.3

11.7

8.1

8.9

10.9

12.3

7.0

3.5

8.1

12.1

12.3

12.2

10.9

–

12.4

7.9

8.8

12.2

12.4

9.3

12.5

12.2

12.3

10.4

Mag 0

in SMC

0.60

0

3.0  2.9

0

0

1.40  1.00

3.1  2.7

0

1.00

h 65

h 59 ¼ h 60

h 62

in SMC

6

6

12, 20

26, 30

20

29.0  6.8

20 0

1 2.60  1.70 Sculptor Galaxy, CH 10, h 61 ¼ h 2345

The Ancient One, h 34

15.00 0

h 57

19.20  5.50

20

121 12, 20

h 56

2

2, 6

4.10

CH 11, h 52, Sailboat Cluster

2, 6

12

6

26, 30

12, 20

2, 6

26, 30

2, 6

2

12

1.30  1.10

Andromeda Galaxy, h 50

companion to Andromeda Galaxy 15.00

0

189.10  61.70

8.5  6.5

0

1.50  1.20

1.9  1.5

h 47

h 46

5.00  3.30 0

in Andromeda Galaxy, h 45

4.20

0

in SMC

0.80

19.5  11.5

companion to Andromeda Galaxy, CH 9, h 44

CH 12

5.00 0

h 40

1.60  1.40 0

h 37

1.40  1.20

12

12 2, 6

h 35

12, 20

12

12

Map no.

8.00  7.00

h 2334

h 33

Name/Notes

1.90  1.60

2.10  1.90

3.2  2.6

0

3.50  2.40

Size

109

271 274 275 278 289 288 292 299 300 296 330 312 315 346 337 362 371 357 366 383 406 411 381 419 393 404 418 410 420 434 428 430 439 454

H II-446

H III-429

h 70

H I-159 *

h 2355

H VI-20 *

h 2356

h 2360

h 2359

H II-214

h 2367

h 2363

H II-210

h 2370

H II-433

h 2375

h 2376

H II-434

h 83

H II-217

h 2381

h 2384

H VIII-64 *

h 2387

H I-54

H II-224 *

h 2385

H II-220

H III-154

h 2392

H II-622

H II-447

h 2394

h 2397

PHE

SCL

CET

CET

TUC

PSC

PSC

SCL

AND

AND

TUC

CAS

TUC

TUC

PSC

CAS

CET

TUC

TUC

CET

TUC

PSC

PHE

TUC

PSC

SCL

TUC

TUC

SCL

SCL

CAS

CET

CET

CET

01 14.4

01 13.8

01 13.1

01 12.9

01 12.2

01 12.1

01 11.0

01 10.6

01 09.4

01 08.6

01 08.3

01 08.3

01 07.9

01 07.4

01 07.4

01 06.4

01 03.4

01 03.3

01 03.2

00 59.8

00 59.1

00 57.8

00 56.3

00 56.2

00 55.4

00 54.9

00 54.0

00 52.8

00 52.8

00 52.7

00 52.1

00 51.1

00 51.0

00 50.8

55 24

31 45

00 15

þ00 59

58 15

þ32 06

þ33 09

30 13

þ35 43

þ39 40

72 53

þ61 35

71 46

69 53

þ32 25

þ62 14

06 20

72 05

70 51

07 35

72 11

þ30 21

52 47

72 29

þ31 40

37 41

72 10

72 50

26 35

31 12

þ47 33

07 04

07 03

01 53

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GC

OC

OC

GX

GX

OC

GX

OC

GC

GX

OC/DN

GX

GX

OC

GX

GX

OC/DN

GX

GC

GX

GX

GX

GX

GX

12.2

11.5

12.5

11.3

12.0

12.2

11.5

12.4

10.1

12.4

11.2

9.3

12.2

12.3

12.2

–

12.2

–

6.8

11.6

10.3

11.2

12.4

9.6

12.4

8.1

11.7p

2.2

8.1

10.9

10.7

12.5

11.8

12.2 0

1.4 0

0

Mirach’s (Beta AND) Ghost/False Comet

1.70  1.40 3.50

1.7  1.5

0

0

2.50  1.50

1.3  1.1

0

26

20

12, 13

12, 13 0

26 4.00  2.90

6 6

2.00  1.80 2.20  1.20

20 2.40  1.30

6 2.00  1.70 h 90

h 88

2.40

2, 6

2, 3 26, 30

in SMC

7.00

26, 30 26, 30

1.30

in SMC

2.60  1.00

2, 3 6

h 86

12, 13

26, 30

26, 30

12

26, 30

6

2.00  1.70

h 82

in SMC

h 80

in SMC

h 79

26

26, 30

4.00

2.50  1.70

7.5

0

14.00

3.0  1.8

0

14.00  11.00

3.0  2.5

0

1.40  1.10

in SMC

6

0

20

26, 30

2.20  1.00

in SMC

19.00  12.90

0.70

26, 30

20

Small Magellanic Cloud

319.10  205.10

13.0 h 74 ¼ h 2354

2, 6 20

h 71

12

12

12

0

0

h 69

h 67

5.10  3.60

2.1  2.0

0

1.50  1.20

1.4  1.2

0

2.20  1.70

110 514 520 521 517 524 533 529 545 547 536 564 559 602 578 584 596 581/M 103

H III-253

H II-461

H III-168

H I-151 *

H II-462

h 118

H II-448

H II-449

H III-171

H III-442

H VII-48 *

h 2421

h 2418

H I-100 *

H II-4 *

h 126

474

H III-251

507

470

H III-250

H II-252

484

h 2406

H III-159

467

H I-108

499

457

H VII-42 *

H III-158

436

H VII-45 *

493

465

h 2404

H III-594

450

H III-440

491

433

h 94

488

460

h 2402

H III-252 *

456

h 2399

h 2407

NGC/M

Herschel

CAS

CET

CET

CET

HYI

CAS

CET

AND

CET

CET

AND

CET

PSC

PSC

CET

PSC

PSC

PSC

PSC

CET

PSC

SCL

PSC

PSC

TUC

PSC

CAS

CAS

TUC

CET

CAS

TUC

TUC

Con

01 33.2

01 32.9

01 31.3

01 30.5

01 29.6

01 29.5

01 27.8

01 26.4

01 26.0

01 26.0

01 25.7

01 25.5

01 24.8

01 24.7

01 24.6

01 24.6

01 24.1

01 23.7

01 23.2

01 22.2

01 21.8

01 21.4

01 20.1

01 19.7

01 19.2

01 19.2

01 19.1

01 15.6

01 15.5

01 15.5

01 15.3

01 14.8

01 14.4

þ60 42

07 02

06 52

22 40

73 33

þ63 18

01 53

þ34 43

01 21

01 20

þ34 44

þ01 46

þ09 32

þ33 27

þ01 44

þ03 48

þ12 55

þ33 15

þ33 28

þ00 57

þ05 15

34 03

þ03 25

þ03 25

58 31

þ03 18

þ58 20

þ58 49

73 20

00 52

þ60 08

73 18

73 17

RA (2000.0) Dec

OC

GX

GX

GX

OC/DN

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

OC

OC

GX

OC

OC/DN

DN

Type

7.4

10.9

10.5

10.8

–

9.5

12.5

12.4

12.3

12.3

12.2

11.4

10.4

12.5

11.7

11.3

11.6

11.3

12.2

12.2

10.4

12.4

11.3

11.7

11.2

12.1

6.4

8.8

11.5

11.6

–

12.5

–

Mag

12, 13

h 106

1.70  1.30

h 128 h 132 6.0

0

4.1  2.0

3.20  2.00

2, 3

12, 13

12, 13

20 0

0

26, 30

2, 3 4.80  3.00

h 124

12, 13 34.00

7.0

0

1.30  1.10

3.3  1.2

6

12, 13 0

0

12, 13

2.6  1.6

1.90  1.80

6

12, 13

6, 12, 13

6

12, 13

12, 13

6, 12, 13

6

6

12, 13

12, 13

0

0

h 120

h 121 2.40  2.10

3.8  2.3

0

0

h 117

2.80

1.4  0.5

0

h 114

h 115 0

h 116

3.4  1.7

2.70  2.40

h 112 0

0

3.70  3.00

2.5

h 108

h 105

3.40  1.10 0

h 103

5.40  3.90

1.4  1.0

20

12, 13

0

0

12, 13

2.9  1.7 7.10  6.30

26, 27

0

0

12, 13

h 99

1.70 1.90  1.40

2, 3 2, 3

26, 30

ET/Owl Cluster, h 97

in SMC

2, 3

20.00

0

26, 30

26, 30

Map no.

5.00

2.00

3.0  2.4

0

4.00

1.0 in SMC

in SMC

15.00 0

Name/Notes

Size

111

685 672 673 692 676 686 681 678 679 680 684 693 691

H II-589

h 2419

H IV-42

H III-459

H II-481

H II-228

H III-175

H II-229

H II-612

H II-859

H II-617

665

H II-588

H I-157

663

H VI-31 *

h 2438

661

637

H VII-49 *

H II-610

650þ651/M76

H I-193 *

659

636

H II-283

H VIII-65 *

642

h 2431

657

641

h 2432

654

632

h 143

H VII-46 *

628/M 74

h 142

h 146

625

615

H II-282 * 630

604

H III-150

h 2426

613

H I-281 *

h 2428

598/M 33

H V-17 *

ARI

PSC

TRI

ARI

AND

ARI

CET

FOR

PSC

PHE

ARI

TRI

ERI

PSC

CAS

TRI

CAS

CAS

CAS

CAS

PER

CET

SCL

PHE

PSC

PSC

SCL

PHE

CET

TRI

SCL

TRI

01 50.7

01 50.5

01 50.2

01 49.8

01 49.7

01 49.4

01 49.2

01 49.0

01 49.0

01 48.7

01 48.4

01 47.9

01 47.8

01 44.8

01 46.0

01 44.2

01 44.2

01 44.1

01 43.7

01 42.9

01 42.3

01 39.1

01 39.9

01 38.7

01 37.3

01 36.7

01 35.6

01 35.1

01 35.1

01 34.5

01 34.3

01 33.9

þ21 46

þ06 09

þ27 39

þ21 58

þ35 47

þ22 00

10 26

23 48

þ05 54

48 39

þ11 32

þ27 26

52 47

þ10 26

þ61 15

þ28 42

þ60 42

þ61 53

þ55 53

þ64 00

þ51 35

07 31

29 54

42 31

þ05 53

þ15 47

39 21

41 26

07 20

þ30 48

29 25

þ30 39

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

OC

OC

OC

OC

PN

GX

GX

GX

GX

GX

GX

GX

GX

DN

GX

GX

11.5

12.3

12.5

11.9

12.4

12.5

12.0

12.4

11.9

12.3

12.5

10.7

11.2

12.2

7.1

12.2

7.9

6.5

–

8.2

11.5

11.5

12.3

12.1

12.4

9.1

11.9

11.1

11.7

12.0

9.9

5.5

h 137

2.70  0.90

6, 12, 13

10.5  9.5 0

h 2436

2.70  1.80

h 156 3.4  2.5

0

0

h 152 2.20  1.10

1.2  0.6

0

0

1.80  1.60

1.9

0

4.50  0.80

h 155 ¼ h 2437

1.70  1.40

4.0  1.0

0

6, 7

12, 13

6, 7

6, 7

6,7

6, 7

12, 13, 20

20, 21

12, 13

20, 26 0

6, 12, 13 2.10  1.80 h 151

26 6, 7 2.10  1.70

6.00  2.40

3.6  3.1

0

6, 12, 13 0

h 150

2, 3 6, 7 2, 3

h 147

1.60  1.30 2.40  1.60

CH 20

6.00

2, 3

2

2, 3

2

12, 13

20, 21

20, 21, 26

15.00

h 145

0

6.00

7.0

0

3.00

1.10

2.8  2.0

0

2.00  1.10

1.4  1.3

0

1.00  0.80

Little Dumbell/Barbell Nebula

20, 21, 26

0

12, 13

20, 21, 26

5.8  1.9 1.60  1.40

12, 13

6

20

6

0

h 144

in Triangulum Galaxy, h 133

2.00

0

h 139 ¼ h 2422

5.50  4.20

0

Triangulum Galaxy, h 131

68.70  41.60

112 777 788 803 807 821 818 835 828 857

H II-223

H II-435

H III-208

H III-151

H I-152

H II-604

H II-483

H II-605

h 2469

877

779

H I-101 *

864

772

H I-112 *

H II-246

743

h 170

H III-457

744

h 171

862

782

h 2454

855

752

H VII-32 *

H II-613

750

H II-222

h 2470

736

H II-221

745

h 2449

755

723

H III-460

H III-265

718

H II-270

748

720

H I-105 *

H III-193

708

H III-565

749

706

H II-596

741

697

H III-179

H II-271

701

H I-62

h 2448

NGC/M

Herschel

ARI

CET

TRI

PHE

FOR

AND

CET

AND

ARI

TRI

ARI

CET

TRI

CET

ARI

CAS

PER

ERI

AND

TRI

TRI

CET

CET

PSC

FOR

ERI

CET

PSC

CET

AND

PSC

ARI

CET

Con

02 18.0

02 15.5

02 14.0

02 13.0

02 12.6

02 10.2

02 09.4

02 08.7

02 08.4

02 04.8

02 03.8

02 01.1

02 00.2

01 59.7

01 59.3

01 58.7

01 58.4

01 57.8

01 57.8

01 57.5

01 56.7

01 56.4

01 56.4

01 56.4

01 55.6

01 54.2

01 53.9

01 53.2

01 53.0

01 52.8

01 51.8

01 51.3

01 51.1

þ14 33

þ06 00

þ27 53

42 04

31 57

þ39 12

10 08

þ38 47

þ11 00

þ28 59

þ16 02

06 49

þ31 26

05 58

þ19 01

þ60 11

þ55 29

57 46

þ37 41

þ33 13

þ33 03

09 04

04 28

þ05 38

29 57

56 41

23 46

þ04 12

13 44

þ36 10

þ06 18

þ22 21

09 42

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

OC

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

Type

11.8

11.0

12.3

11.9

12.4

12.2

12.2

12.4

10.8

12.5

12.5

21.1

11.5

11.2

10.3

–

7.9

11.7

5.7

12.0

12.2

12.6

12.6

11.3

12.5

12.4

12.5

11.7

11.2

11.9

12.5

12.0

12.2

Mag h 160 ¼ h 2442

2.60  1.40

0

h 177 ¼ h 2447 h 169 h 175

3.30  1.10 1.50 1.60  1.30 75.0

h 185 h 190

h 197

2.50  1.60

h 206 h 210

2.40  1.90

4.7  3.5

0

0

2.60  1.00

0.8

0

1.50  1.30

h 200 ¼ h 2464

1.30  1.10

2.9  1.2

0

h 194

h 193 0

h 191 2.40  1.70

1.8  1.3

0

0

1.6  1.4

3.00  1.30

2.50  2.00 0

h 182

4.10  1.20 0

h 183

7.20  4.30

7, 13

13

6, 7

20, 21, 26

20, 21

2, 6, 7

13, 21

2, 6, 7

7, 13

6, 7

7, 13

13

6, 7

12, 13

2, 3 6, 7, 12, 13

h 181

7.00

5.0

2, 3

26, 27

2, 6, 7

6, 7

6, 7

12, 13

0

2.40  2.10

0

CH 13, h 174

h 176

2.30  1.10

12, 13

20, 21 12, 13

1.9  1.4 h 172

26, 27

20, 21

12, 13

12, 13, 20

3.00  2.90

h 166 ¼ h 2444

h 164

2, 6, 7

12, 13

6, 7

12, 13, 20

Map no.

0

0

1.30  0.80

1.5  1.3

0

2.30  2.20

4.7  2.4

0

h 165 ¼ h 2443

h 159

0

h 161

3.00  2.50

1.9  1.5

0

0

4.00  1.30

Name/Notes

Size

113 1024

990

H III-557

H II-592

991

H III-434

1022

982

H III-573

H I-102 *

978

h 234

1031

972

H II-211

987

969

h 231

h 2490

986

h 2487

H III-161

956

949

H I-154 957

958

H II-237

h 228

955

H II-278

h 227

945

H II-487

ARI

932 941

H II-489

936

H III-261

CET

925

H IV-23 *

ARI

CET

TRI

HOR

ARI

CET

AND

TRI

ARI

TRI

FOR

PER

AND

TRI

CET

CET

CET

CET

TRI

ARI

AND

FOR

CAS

CET

H III-177

908

H I-153 *

AND

918

891

H V-19 *

PER

TRI

h 221

884

H VI-34 *

910

890

H II-225

CET

CET

H III-571

899

h 2476

886

895

H II-438

FOR

PER

922

897

h 2475

H III-239

869

H VI-33 *

CET

h 214

881

H II-436

02 39.2

02 38.5

02 36.8

02 36.6

02 36.4

02 35.5

02 35.4

02 34.8

02 34.2

02 34.1

02 33.6

02 33.6

02 32.4

02 30.8

02 30.7

02 30.6

02 28.6

02 28.5

02 27.9

02 27.6

02 27.3

02 25.9

02 25.4

02 25.1

02 23.5

02 23.1

02 22.6

02 22.4

02 22.0

02 21.9

02 21.6

02 21.1

02 19.0

02 18.7

þ10 51

06 40

þ33 19

54 52

þ11 39

07 09

þ40 57

þ32 52

þ29 19

þ32 58

39 02

þ57 32

þ44 39

þ37 08

02 57

01 07

10 32

01 09

þ20 19

01 09

þ33 35

þ18 30

þ41 50

24 47

þ63 47

21 14

þ42 21

þ57 07

þ33 16

20 48

05 31

33 42

þ57 09

06 35

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

OC

GX

GX

GX

GX

OC

GX

12.3

11.3

12.5

12.5

12.5

11.7

12.5

12.2

11.3

12.3

10.8

7.6

8.9p

11.6

12.2

12.1

12.1

12.2

12.5

10.2

9.9

12.4

12.2

11.8

–

10.2

10.1

6.1

11.3

12.5

11.7

12.0

5.3

12.5 18.0 0

0

h 239 h 238

1.80  1.50

h 237 h 244 h 243

2.40  2.20 3.90  1.50

1.9  1.1

1.60  1.10

0

0

h 236 3.00  2.70

1.5  0.6

0

0

1.30  1.00

3.3 1.6

0

1.70  1.00

4.0  3.2

0

10.00

6.0  1.0

0

h 232

h 226 0

h 230

2.9  0.9

3.00  1.60

h 229

2.90  0.90 0

h 225 ¼ h 2480

2.30  2.20 0

h 224

0

2.70  1.80

1.9  1.6

0

7, 13

13

7

26, 27

7, 13

13

2, 6, 7

7

7

7

20, 21, 26

2, 3

2, 6, 7

6,7

13

13

13, 21

13

7

13

6, 7

4.70  4.10

h 223

0

h 222

7, 13

3.50  2.00 10.5  5.9

2, 6, 7

1.60 0

2, 3 21

h 2478

2.00  1.60

14.0

21

2, 6, 7

0

h 218

2, 3

6,7

21

13

20, 21

2, 3

13

6.10  2.70

11.70  1.60

h 217 Double Cluster, h 212

0

h 219

Double Cluster, h 207

h 211

18.00

2.5  1.7

0

1.80  1.30

3.6  2.6

0

2.10  1.30

0

2.30  1.50

114 1070 1058

H II-273

H II-633

1106 1122 1134 1129 1140 1153 1162 1156 1161 1172 1167 1187

h 268

H II-601

H II-254

H II-602

H II-470

H II-274

H III-469

H II-619

H II-239

H II-502

H III-178

H III-245

ERI

PER

ERI

PER

ARI

ERI

CET

ERI

PER

ARI

PER

CET

FOR

ERI

FOR

CET

PER

CET

TRI

ARI

PER

1060

H III-162

CET

1056

H III-584

CET

CAS

1090

1068/M 77

h 262

1087

1027

H VIII-66 *

CET PER

H II-465

1039/M 34

h 248

H II-466

1055

H I-1 *

CET

CET

1097

1052

H I-63 *

1084

1045

H II-488

PER

CET

H V-48

1023

H I-156 *

H I-64 *

1035

H II-284

CET

ARI

1073

1032

H II-5

1079

1012

H III-152

PER

H III-455

1003

H II-238

Con

h 2494

NGC/M

Herschel

03 02.6

03 01.7

03 01.6

03 01.2

02 59.7

02 58.9

02 58.1

02 54.6

02 54.5

02 53.6

02 52.8

02 50.6

02 46.6

02 46.4

02 46.3

02 46.0

02 43.7

02 43.7

02 43.5

02 43.3

02 43.2

02 42.9

02 42.7

02 42.7

02 42.0

02 41.8

02 41.1

02 40.4

02 40.4

02 39.5

02 39.4

02 39.3

02 39.3

22 52

þ35 12

14 50

þ44 55

þ25 14

12 24

þ03 22

10 02

þ41 35

þ13 00

þ42 12

þ41 41

00 15

00 30

30 17

07 35

29 00

þ01 23

þ37 21

þ04 58

þ32 24

þ28 33

00 01

þ61 33

þ42 47

þ00 26

08 15

11 18

þ39 04

08 08

þ01 06

þ30 09

þ40 52

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

OC

GX

GX

GX

GX

GX

GX

GX

GX

Type

10.6

12.4

11.9

11.1

11.7

12.5

12.5

12.5

11.9

12.3

12.2

12.5

11.8

10.8

9.5

10.7

11.5

10.8

11.2

12.0

12.0

12.5

8.9

6.7

5.2

10.6

10.5

12.4

9.5

12.2

11.8

12.2

11.3

Mag h 241 h 246 h 249 h 242

7.40  2.50

13

h 265 h 266

h 276

1.20  0.70

4.2  3.2

0

0

h 2504

21

7

13, 21

h 280

2.30  1.70 3.30  2.30

7 7

h 277

2.80  2.00

13

13

13, 21

7

2.60  1.70

1.4

h 2502

h 275 ¼ h 2500

1.80  1.00 0

h 271

2.90  2.10

2.5  0.9

7, 13

7 0

0

7

1.3  1.0

1.80  1.30

13

13

21

13

0

0

3.9  2.3

3.90  1.80

h 2496

h 264 0

0

9.40  6.60

2.8  1.4

0

21 0

4.9  4.3

13

7

13

5.50  3.10

h 255

7

0

0

2.50

2.3  1.9

0

h 263

h 257

0

h 256

2.30  1.70

2.4  1.1

0

0

7

2, 3

15.0 7.10  6.00

2, 6, 7

13

13

13, 21

7

13

13

7

2, 6, 7

Map no.

0

25.00

7.6  2.7

0

h 258

h 254 ¼ h 2439

0

h 253 ¼ h 2491

2.80  2.00

1.6  1.2

0

0

2.2  0.6

0

0

2.5  1.1 3.40  1.10

h 240

0

4.30  1.30 0

Name/Notes

Size

115

1232 1249 1241 1220 1261 1248 1253 1245 1184

H II-258

h 2514

H II-286

h 287

h 2517

H III-443

H IV-17

H VI-25 *

H II-704

h 2537

1351

1336

H I-60

1344

1332

H III-197

h 2544

1320

H IV-77

H I-257

1325

h 2535

1339

1326

h 2529

1341

1317

h 2527

h 2538

1316

H I-106

h 2540

1310 1309

h 2524

1300

1217

h 2508

1313

1208

H II-285

h 2522

1209

H II-504

h 2528

1186

H IV-43

1288

1201

H I -109

1291 ¼ 1269

1200

H II-475

h 2521 ¼ h 2518

1199

H II-503

h 2520

1169

H II-620

FOR

FOR

FOR

FOR

FOR

ERI

ERI

ERI

FOR

FOR

FOR

ERI

FOR

ERI

RET

ERI

FOR

CEP

PER

ERI

ERI

HOR

PER

ERI

HOR

ERI

FOR

ERI

ERI

PER

FOR

ERI

ERI

PER

03 30.5

03 28.3

03 28.1

03 28.0

03 26.6

03 26.3

03 24.8

03 24.4

03 23.9

03 22.8

03 22.7

03 22.1

03 21.0

03 19.7

03 18.3

03 17.3

03 17.2

03 16.6

03 14.7

03 14.1

03 12.8

03 12.3

03 11.7

03 11.3

03 10.1

03 09.8

03 06.2

03 06.2

03 06.0

03 05.5

03 04.1

03 03.8

03 03.6

03 03.6

34 52

31 04

32 17

37 09

35 44

21 20

03 01

21 33

36 28

37 06

37 12

15 24

37 08

19 25

66 30

41 08

32 35

þ80 48

þ47 15

02 49

05 13

55 13

þ53 20

08 55

53 21

20 35

39 01

09 32

15 37

þ42 50

26 04

11 59

15 37

þ46 23

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GC

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

11.5

10.4

11.5

11.5

12.1

10.3

12.5

11.4

10.6

11.1

8.4

11.5

12.1

10.3

9.1

8.5

12.1

12.5

8.4

11.7

12.5

8.3

11.8

12.2

11.5

9.8

12.4

12.5

11.4

11.7

10.7

12.5

11.4

11.6 0

0

0

2.80  1.70

4.8  3.1

21

3, 7

21 0

1.50  1.10 0

21

0

h 2542

21

2.10  1.50 1.2  1.1

21

4.50  1.40 0

13

1.90  0.70

21 21

4.80  1.60

h 2534

3.90  2.90

21 21

Fornax A

11.00  7.20

13, 21

21

13, 21

26, 27, 30

21

21

1

2.80  2.40

h 2523

0

2.30  2.20

1.9  1.5

0

6.20  4.10

9.2  7.2

0

11.00  9.50

2.3  1.9

0

h 290

3, 7

2.80  0.60

10.0

13

0

13

5.30  2.30

1.2  1.0

h 292

26, 27 0

6.80 0

2, 3

2.00

26, 27 13

3.40  1.60

h 289 ¼ h 2510

4.70  2.50

21 21

h 2509

13, 21 13

7.40  6.50

h 285 ¼ h 2507

7

21

13, 21

13, 21

1, 2, 7

1.80  1.30

1.90  0.90

2.2  1.1

0

h 286

h 281

0

h 283

3.6  2.1 3.20  1.20

h 2506

h 282

h 279

0

0

2.90  2.30

2.3  1.7

0

4.00  2.60

116 1354 1357 1365

H III-487

H II-290

h 2552

1415 1417

H II-455

1407

H I-107 *

H II-267

1400

H II-593 1412

1406

h 2572

1419

1401

H III-247

h 2574

1404

h 2571

h 2576

1411

h 2573

FOR

1395

H I-58 1399

1385

H II-263

1393

1383

h 2562

h 2569

1376

H II-288

H III-451

ERI

1387

h 2564

FOR

ERI

ERI

ERI

FOR

ERI

ERI

FOR

ERI

FOR

HOR

ERI

FOR

ERI

ERI

FOR

ERI

1379 1377

H III-961

FOR

FOR

ERI

FOR

FOR

ERI

PER

ERI

FOR

ERI

ERI

ERI

PER

FOR

Con

h 2561

1375

H III-559 1374

1370

H II-262

h 2558

1371

H III-857

h 2557

1359 1366

h 2550

1358

1353

H III-246

1348

1342

H VIII-88 *

H VIII-84

1350

h 2545

H III-446

NGC/M

Herschel

03 42.0

03 41.0

03 40.6

03 40.6

03 40.2

03 39.5

03 39.4

03 39.4

03 38.9

03 38.8

03 38.6

03 38.5

03 38.5

03 37.5

03 37.6

03 37.1

03 37.0

03 36.7

03 36.1

03 35.3

03 35.2

03 35.2

03 35.0

03 33.9

03 33.8

03 33.8

03 33.7

03 33.6

03 33.2

03 32.4

03 32.1

03 31.6

03 31.1

04 42

22 34

37 31

26 13

18 35

18 41

31 19

22 44

35 35

44 05

18 26

35 27

23 02

24 30

18 20

05 03

35 31

20 54

35 27

35 14

35 16

20 22

24 56

31 12

19 29

þ51 26

05 05

36 08

13 40

15 13

20 49

þ37 20

33 38

RA (2000.0) Dec

GX

GX

GX

GX/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GC

GX

GC

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

OC

GX

Type

12.1

11.9

12.5

12.5

9.7

10.9

11.7

12.1

10.0

11.3

12.0

9.4

9.8

10.9

12.5

12.1

10.8

12.4

10.7

11.0

12.2

12.4

10.7

11.0

12.0

–

12.1

9.5

11.6

12.3

11.5

6.7

10.4

Mag

21

h 2566

0

2.30  1.20

3.6  1.7

0

0.90

1.8  0.7

0

h 306

h 2575

h 2570 0

h 2567 4.60  4.30

2.5  2.1

0

0

3.90  0.70

2.4  0.6

13

21

21, 27

21

13, 21

13, 21

21

21

21, 27 0

3.30  3.00 0

21, 27

1.80  1.40 h 2568

21, 27 13, 21

6.9  6.5

1.70  1.30

21

21 0

0

h 2565

h 2563 5.00  4.50

3.6  2.2

0

0

13, 21

2.10  1.90 1.90  0.80

21, 27 13

2.80  2.60 h 303

21 21

1.80  0.90

2.4  2.3

0

0

h 2560

21

2.3  0.9 2.70  2.40

21

21

21

13, 21

3

13

21

13, 21

13, 21

0

h 2554

1.50  1.00 0

h 2555

5.60  3.90

h 302

h 2553

0

0

h 2548

2.10  0.90

2.5  1.5

0

6.00

2.1  1.4

0

11.00  6.20

3.2  2.4

0

h 2547

2.30  0.80 0

h 2546

3.40  1.40 21

21 21

h 301

Map no.

17.00

Name/Notes

5.90  3.10

Size

117

1426

H III-248

1521 1527

1501

H IV-53 *

h 2612

1518

h 2611

h 2616

1507

H II-279

1516

1496

h 310

H III-499

1515

h 2609

1502

1512

h 2607

H VII-47 *

1510

h 2606

1494

h 2601 1511

1493

h 2600

1491

1487

h 2597

H I-258

1482

H III-962

h 2608

1483 1490

1444

H VIII-80 *

h 2595

1461

H II-460

h 2599

1460

H II-459 1453

1452

H II-458 ¼ H II-594

H I-155

1440

H III-249

h 2587

1466 1439

h 2590

1436

1421

H II-291

1457

1427

h 2579

h 2581 ¼ h 2582

1425

H II-852

h 2586 ¼ h 2585

1433

h 2580

HOR

ERI

ERI

CAM

CAM

ERI

ERI

PER

DOR

HOR

HOR

PER

HYD

HOR

HOR

ERI

ERI

RET

HOR

PER

ERI

ERI

ERI

ERI

ERI

ERI

HYD

HOR

ERI

ERI

ERI

FOR

FOR

HOR

04 08.4

04 08.3

04 08.1

04 07.7

04 07.0

04 06.8

04 04.5

04 04.4

04 04.1

04 03.9

04 03.5

04 03.4

03 59.5

03 57.7

03 57.5

03 55.8

03 54.7

03 53.5

03 52.7

03 49.4

03 48.5

03 46.4

03 46.1

03 45.4

03 45.0

03 44.8

03 44.5

03 44.5

03 43.6

03 42.8

03 42.5

03 42.3

03 42.2

03 42.0

47 53

21 03

08 53

þ62 20

þ60 55

21 11

02 11

þ52 37

54 06

43 21

43 25

þ51 19

67 38

48 54

46 12

42 22

20 30

66 02

47 29

þ52 40

16 24

03 58

36 41

18 38

18 16

21 55

71 41

44 38

35 51

22 07

13 29

35 25

29 54

47 13

GX

GX

GX

OC

PN

GX

GX

OC

GX

GX

GX

DN

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

GX

10.7

11.6

11.8

6.9

11.5

11.7

12.3

9.6

11.3

10.2

12.4

–

11.0

11.6

11.1

11.6

12.2

12.4

12.3

6.6

11.8

11.6

12.5

11.9

11.6

11.3

11.4

10.7

11.7

11.3

11.4

10.8

10.6

9.8 0

h 2577 h 2578

2.60  1.60

21, 27

h 2583

2.20  1.60

1.6  1.4 0

Oyster Nebula

2.7  1.6

3.90  1.50

0

h 2610

1.40  0.90 0

Golden Harp Cluster

20.00

21, 27

21

13, 14

2, 3

21 2, 3

13, 14

3

0.90

0

27

2.90  1.40

3.6  1.0

0

3.00

5.4  1.3

0

21, 27 0

3.2  1.8

21, 27

3

26, 27, 30

21, 27

8.90  5.60

0

21, 27

21, 27

21

26, 27, 30

21, 27

3

13, 21

13

21, 27

13, 21

13, 21

21

0

0

25.00

3.5  1.3

0

3.30  2.00

2.8

0

2.40  1.70

2.4  1.4

0

1.30  1.10 h 2594

h 308

4.00 0

h 2588

3.00  0.90 0

h 309

0

2.40  1.90

1.4  1.0

0

2.80  1.50

h 2584

2.40  2.20

1.9

0

26, 27, 30

21, 27

3.1  2.0 7.60  1.70

21

13, 21

21, 27

21

21, 27

0

0

3.4  0.8

0

0

3.80  2.60

5.8  2.5

0

6.50  5.90

118 1569 1589 1600 1617 1582

H II-768

H I-158

h 2651

H VIII-70

1587

H II-8

H II-7

1579

H I-217

1566

h 2635

1596

1550

H II-464

1581

1559

h 2634

h 2648

1553

h 2630

h 2642

1549

h 2629

1572

1528

H VII-61 *

1570

1546

h 2628

h 2639

1535

H IV-26 *

h 2637 ¼ h 2638

1537

h 2624

1574

1557

h 2633

1567

1543

h 2627

h 2640

1532

h 2621

h 2636

1531

h 2620

1558

1513

H VII-60 *

1545

1533

h 2622

H VIII-85 *

1514

H IV-69

h 2632

NGC/M

Herschel

PER

DOR

ERI

TAU

CAM

TAU

PER

DOR

DOR

CAE

CAE

RET

CAE

PER

CAE

DOR

TAU

RET

DOR

DOR

PER

DOR

ERI

ERI

HYD

RET

ERI

ERI

PER

DOR

TAU

Con

04 32.0

04 31.7

04 31.7

04 30.8

04 30.8

04 30.7

04 30.2

04 27.6

04 24.7

04 22.6

04 22.1

04 22.0

04 21.1

04 20.9

04 20.3

04 20.0

04 19.6

04 17.6

04 16.2

04 15.7

04 15.4

04 14.6

04 14.2

04 13.7

04 13.3

04 12.8

04 12.1

04 12.0

04 10.0

04 09.9

04 09.2

þ43 51

54 36

05 05

þ00 51

þ64 51

þ00 40

þ35 16

55 02

54 56

40 36

43 38

56 58

48 15

þ50 15

45 02

54 56

þ02 26

62 47

55 47

55 36

þ51 14

56 04

12 44

31 39

70 25

57 44

32 52

32 51

þ49 31

56 07

þ30 47

RA (2000.0) Dec

OC

GX

GX

GX

GX

GX

DN

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

OC

GX

PN

GX

OC/NE

GX

GX

GX

OC

GX

PN

Type

7.0

10.5

11.0

12.0

11.2

11.7

–

11.1

12.5

12.5

12.3

10.3

11.5

6.2

12.5

9.4

12.1

10.4

9.0

9.6

6.4

11.0

9.6

10.5

–

10.3

9.8

11.7

8.4

10.7

10.9

Mag

21

4.5  2.8

h 315

21, 27 21, 27

7

12.0  8.0

h 319

2.50  1.70

3, 7

0

24.0

27

4.30  2.10

13, 14

1, 2, 3 13, 14

h 318

3.20  1.00

3.7  1.8

0

0

1.70  1.40

13, 14

27 0

h 316

27 3.70  0.90

1.8  0.7

0

0

1.5  1.2

2.40  1.20

26, 27, 30

21, 27

3, 7

0

0

4.00  3.60

1.3

0

12.00

2.5  1.0

27

13, 14 0

0

21, 27

2.2  1.9

8.20  6.50

26, 27, 30 0

0

3.50  2.00

27

27 0

3

4.90  4.10 0

26, 27

18.00

13, 14, 21

3.20  1.90

0.8

0

21

26, 27, 30

3.90  2.60

10.0

26, 27, 30

0

11.6  3.4 3.80  2.80

0

21

0

Lassell’s Most Extraordinary Object, h 2618

3, 7

12.0 1.20  0.90

26, 27, 30

7

Map no.

0

0

Crystal Ball Nebula, h 311

2.20 2.80  2.30

Name/Notes

Size

119 1743

1703

h 2678

1735

1684

H II-528

h 2699

1727

h 2690

h 2696

1718

h 2688

1731

1714

h 2686

1732

1712

h 2685

h 2691

1664

H VIII-59 *

h 2694

1679

1704

h 2683 1711

1698

h 2677

h 2666

1702

h 2680

h 2684

1663

H VIII-7

DOR

1688 1662

h 2671

1695

h 2673

H VII-1

DOR

1659

H III-589

DOR

DOR

DOR

DOR

DOR

ORI

DOR

DOR

DOR

DOR

AUR

MEN

CAE

DOR

DOR

MEN

ORI

ORI

ERI

TAU

ERI

DOR

1653

1672

h 2665

ERI

1647

1638

H II-525

ERI

H VIII-8 *

1637

H I-122

PER

ERI

MEN

ERI

ERI

DOR

PER

CAE

H II-526

1624

H V-49

1625

h 322 1651

1620

H II-514

1635

1641

h 2656

H II-515

1605

H VI-26

h 2662

1616

h 2650

04 54.0

04 53.9

04 53.4

04 52.9

04 52.8

04 52.5

04 52.2

04 52.2

04 52.1

04 51.3

04 51.1

04 50.5

04 50.0

04 49.7

04 49.4

04 49.3

04 48.6

04 48.5

04 48.4

04 47.6

04 46.5

04 46.0

04 45.8

04 45.7

04 41.6

04 41.4

04 40.4

04 40.1

04 37.5

04 37.1

04 36.6

04 36.1

04 35.0

04 32.7

69 12

67 07

66 56

68 40

59 45

03 06

69 21

67 04

66 56

69 28

þ43 42

70 00

31 59

69 45

69 10

69 51

þ13 10

þ10 56

59 48

69 24

04 47

þ19 04

02 25

59 15

01 49

02 51

þ50 27

00 33

70 35

03 18

00 09

65 46

þ45 15

43 43

OCþDN

OCþDN

OCþDN

OC

GX

GX

OCþDN

OC

OCþDN

OCþDN

OC

OC

GX

OC

DN

OC

OC

OC

GX

OC

GX

OC

GX

GX

GX

GX

OC/DN

GX

GC

GX

GX

OC

OC

GX

–

10.8

9.9

12.3

11.2

12.0

11.1

12.3

11.6

–

7.6

10.1

11.4

11.5

12.1

12.5

14.5

6.4

11.6

12.2

12.5

6.4

11.9

9.7

12.0

10.8

11.8

12.5

12.3

12.3

12.4

–

10.7

12.5

0

2.7  2.0

2.20  1.70

in LMC

27, 30, 32

27, 30, 32

in LMC 2.20

1.6

27, 30, 32 0

27, 30, 32

26, 27, 30

13, 14

8.00

0.9

0

in LMC

h 334

2.50 2.90  2.60

in LMC

2.00

27, 30, 32

27, 30, 32 27, 30, 32

in LMC

1.20

3, 7 27, 30, 32

in LMC

2.50

27, 30, 32

21

27, 30, 32

18.00

2.40

in LMC

in LMC

1.70 0

in LMC

1.60

27, 30, 32

7, 13, 14 27, 30, 32

7, 13, 14

26, 27, 30

27, 30, 32

13, 14

in LMC

h 332

in LMC

h 331

7, 13, 14

1.00

0

0

0

9.00

12.00

2.4  1.9

0

1.50

1.5  1.1

0

40.00

1.5

13, 14

26, 27, 30

6.70  5.60 0

13, 14

1.80  1.20

3, 7 13, 14

h 327

13, 14

27, 30, 32

13, 14

13, 14

3.30  2.70

h 325

h 321

26, 27, 30

3, 7

21, 27

3.00

1.40  1.30

2.5

0

2.10  0.50

2.9  1.0

0

9.00  6.00

5.0

0

1.80  0.90

120 1814

1806

h 2745

h 2748

1804

h 2742

1823

1801

h 2739

h 2758

1744

h 2692

1810

1726

h 341

1796

1795

h 2738

h 2746

1793

h 2736

h 2735

1786

h 2729

1708

1787

h 2731

h 337

1783

h 2726

1815

1774

h 2723

h 2753

1769

h 2716

1809

1782

h 2727

1805

1770

h 2715

h 2747

1700

H IV-32

h 2741

1763

h 2711

1766

h 2717

1772

1755

h 2706

h 2722

1747

h 2701

1767

1756

h 2707

1761

1754

h 2708

h 2710

1705

h 2679

h 123

NGC/M

Herschel

DOR

MEN

DOR

DOR

CAM

MEN

DOR

DOR

DOR

DOR

DOR

LEP

ERI

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

ERI

DOR

DOR

DOR

DOR

MEN

DOR

DOR

DOR

MEN

PIC

Con

05 03.8

05 03.5

05 03.1

05 02.7

05 02.6

05 02.3

05 02.2

05 02.0

05 01.9

05 00.9

05 00.5

05 00.0

04 59.7

04 59.5

04 59.4

04 59.1

04 59.1

04 58.9

04 57.8

04 57.7

04 57.6

04 57.0

04 56.9

04 56.8

04 56.7

04 56.4

04 56.3

04 55.8

04 55.0

04 54.9

04 54.6

04 54.4

04 54.2

67 17

70 21

66 22

61 08

þ52 53

70 37

66 06

69 34

67 59

69 05

69 38

26 01

07 45

69 48

69 33

67 45

65 44

66 00

67 15

66 28

69 23

68 25

04 52

66 24

69 34

66 30

69 24

70 14

68 11

67 11

69 15

70 27

53 22

RA (2000.0) Dec

OCþDN

OC

OC

GX

OC/NE

OC

OC

GX

GC

OC

OC

GX

GX

GC

OC

GC

OC

GC

OC

OCþDN

OCþDN

OCþDN

GX

DN

OCþDN

OCþDN

OCþDN

OC

OC

OCþDN

OC

GC

GX

Type

9.0

12.1

11.9

12.1

–

12.4

10.6

12.5

11.1

11.9

12.2

11.1

11.7

12.4

12.4

10.9

10.9

10.9

10.8

–

10.5

9.0p

11.2

–

11.0

9.9

10.6

12.2

9.9

9.4

12.2

12.0

11.8

Mag

in LMC in LMC in LMC in LMC in LMC in LMC

0.70 0

1.20 1.50 0

in LMC in LMC in LMC

0

in LMC

1.20

in LMC in LMC Identical triple clusters plus nebulosity within LMC

1.20 0.90 1.00

1.8  1.0

0

20.00

in LMC

3.2  0.8 2.20

0

in LMC

2.20 0

in LMC

1.00 0

in LMC

0

2.20

7.4  3.5

0

1.70  1.40

1.6

1.6

1.30

in LMC

23.00 0

in LMC

3.00

27, 30, 32

27, 30, 32

27, 30, 32

26, 27, 30

3

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

21

13, 14

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32 27, 30, 32

27, 30, 32

27, 30, 32

in LMC

in LMC

1.20 –

in LMC

1.60

13, 14

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27

Map no.

1.80

h 336

3.30  2.10

5.0  3.0

1.6

2.6

0

0

in LMC

1.10 –

in LMC

Name/Notes

–

1.90  1.40

Size

121

1847 1844 1848 1846 1808 1778 1850 1852 1854 1856

h 2773

h 2776

h 2774

h 2740

H VIII-61

h 2780

h 2781

h 2782 ¼ h 2783

h 2784

1845

h 2770

h 2775

1831

h 2759

1824

1839

h 2768

h 2755

1784

h 2719

1788

1834

h 2764

H V-32 *

1836

h 2766

1800

1779

H III-500

1840

1835

h 2763

h 2732

1792

h 2730

h 2771

1829

h 2760

1818

h 2749 1758

1828

h 2761

1837

1750

H VIII-43

H VII-21

1820

h 2754

h 2769

1816

h 2750

DOR

DOR

DOR

DOR

AUR

COL

DOR

MEN

DOR

DOR

DOR

ORI

MEN

COL

MEN

DOR

DOR

LEP

DOR

DOR

ERI

DOR

COL

DOR

MEN

TAU

DOR

DOR

TAU

DOR

DOR

05 09.4

05 09.1

05 09.0

05 08.5

05 08.1

05 07.7

05 07.6

05 07.3

05 07.2

05 06.9

05 06.9

05 06.9

05 06.4

05 06.4

05 06.3

05 06.1

05 05.9

05 05.4

05 05.3

05 05.3

05 05.3

05 05.2

05 05.2

05 04.7

05 04.7

05 04.4

05 04.2

05 04.1

05 03.9

05 03.8

05 03.8

69 08

68 51

67 47

68 46

þ37 03

37 31

67 28

71 11

67 19

68 59

59 43

03 21

71 49

31 57

70 28

64 55

68 37

11 52

69 13

68 37

09 09

69 24

37 59

68 03

70 42

þ23 46

66 24

69 23

þ23 39

67 17

67 17

OC

GC

OC

OC

OC

GX

OC

OCþDN

OC

OC

GX

DN

OC

GX

OC

OC

OCþDN

GX

OC

OC

GX

GC

GX

OCþDN

OCþDN

OC

OC

OC

OC

OC

OCþDN

10.1

10.4

12.0

9.0

7.7

9.9

11.3

9.7

12.1

11.1

12.5

–

–

12.5

10.2

11.1

11.8

11.7

11.8p

12.2

12.1

11.3

10.0

8.0p

10.6

7.0

9.7

12.5

–

9.0

9.0

in LMC

in LMC

in LMC

20.00

h 347

5.00  3.00

in LMC in LMC

1.30

in LMC

0

in LMC in LMC

– 1.80

1.8

in LMC

3.40

8.0

0

h 344

in LMC 6.50  3.90

in LMC

– 2.80

1.0

0

3.20  0.80

in LMC

0.60

2.0  1.1

0

in LMC

3.90 0

in LMC

–

4.10  2.60

in LMC

0.80 –

h 345 ¼ h 2714

2.50  1.40

1.2

0

in LMC

in LMC

2.10 5.20  2.60

in LMC

40.0 1.30

0

in LMC

0.7 3.40

Identical triple clusters plus nebulosity within LMC

Identical triple clusters plus nebulosity within LMC

0

25.00  12.00

–

1.00

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

7

21

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

26, 27, 30

14

27, 30, 32

21

27, 30, 32

27, 30, 32

27, 30, 32

14, 21

27, 30, 32

27, 30, 32

14

27, 30, 32

21

27, 30, 32

27, 30, 32

7

27, 30, 32

27, 30, 32

7

27, 30, 32

27, 30, 32

122

1802 1860 1807 1859 1863 1817 1832 1870 1872 1874 1876 1877 1866 1873 1871 1869 1851 1868 1885 1882 1894 1898 1892 1903 1916 1914 1901 1902 1910 1913 1922 1919

H VIII-41

h 348

h 2786

h 2791

H VII-4 *

H II-292

h 2799

h 2801

h 2803

h 2804

h 2805

h 2793

h 2802

h 2800

h 2798

h 2777

h 2796

h 2814

h 2809

h 2818

h 2822

h 2815

h 2825

h 2829

h 2830

h 2824

h 2823

h 2827

h 356

h 374

h 2832

1858

h 2785

h 2787

NGC/M

Herschel

DOR

DOR

DOR

DOR

DOR

DOR

MEN

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

COL

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

LEP

TAU

DOR

DOR

TAU

DOR

TAU

DOR

Con

05 20.0

05 19.7

05 18.4

05 18.1

05 18.1

05 17.8

05 17.6

05 17.5

05 17.2

05 17.1

05 16.7

05 15.7

05 15.2

05 15.0

05 14.5

05 14.1

05 13.8

05 13.7

05 13.7

05 13.5

05 13.2

05 13.2

05 13.2

05 13.0

05 13.0

05 12.1

05 12.1

05 11.4

05 11.4

05 10.7

05 10.4

05 10.2

05 09.7

66 55

69 29

69 33

69 13

66 37

68 26

71 14

69 22

69 18

64 57

69 36

69 27

66 07

68 58

63 57

40 03

67 23

67 28

67 20

65 28

69 23

69 23

69 23

69 20

69 08

15 41

þ16 42

68 47

65 13

þ16 32

68 46

þ24 06

68 54

RA (2000.0) Dec

OCþDN

OC

OC

OC

OC

OC

OCþDN

OC

OC

GX

OC

OC

OC

OC

GC

GC

OCþDN

OCþDN

OCþDN

OC

OCþDN

OCþDN

OCþDN

OCþDN

OC

GX

OC

OC

OC

OC

OC

OC/NE

OCþDN

Type

–

11.5

11.1

11.2

11.8

–

12.0

10.4

11.9

12.1

11.9

12.2

12.3

12.0

11.6

7.1

–

10.1

10.4

9.7

12.0p

11.7

9.0p

11.0

11.3

11.3

7.7

11.0

12.3

7.0

11.0

–

9.9

Mag

in LMC h 349

0.50 20.00

in LMC

0

in LMC in LMC

1.20 0

in LMC in LMC in LMC in LMC

0

0.60 0

1.70

0.5

8.5

in LMC

in LMC 1.60

40.0

in LMC

2.20 0

in LMC

–

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32 27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

1.00

in LMC

21 27, 30, 32

2.90  0.80

–

in LMC

in LMC

0.80 0.8

in LMC

12.0 3.90

0

27, 30, 32

27, 30, 32

14.00

2.0

27, 30, 32

0

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

3.50 in LMC

in LMC

4.5

in LMC

1.00 3.00

in LMC

1.00 –

in LMC

0.50

27, 30, 32

14, 21 27, 30, 32

in LMC

2.60  1.70

7, 14

27, 30, 32

7, 14 27, 30, 32

27, 30, 32

7

27, 30, 32

in LMC

in LMC

in LMC

Map no.

2.00

0

Name/Notes

12.00

0.80

20.0

–

Size

123

1962 1970 1967 1969 1971 1947 1966 1968 1987

h 2867

h 2869

h 456

h 2872

h 2875

h 2855

h 2868

h 2870

h 2885

1986

1955

h 2863

1984

1951

h 2858

h 2883

1930

h 2836

h 2882

1909

H V-38

1983

1883

H VII-34

2000

1959

h 2865

h 2881

1948

h 2889

1953

1893

h 351

h 2856

1940

h 2847

h 2862

1888

H II-289

1943

1944

h 2852

1896

1925

h 2837

H VIII-4

1938

h 2848

h 2850

1923 1891

1928

h 2839

h 2835

1926

h 2838

h 2811

1857

H VII-33 *

MEN

DOR

DOR

MEN

MEN

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

DOR

PIC

ORI

AUR

MEN

DOR

DOR

TAU

MEN

AUR

DOR

LEP

MEN

DOR

MEN

COL

DOR

DOR

DOR

AUR

05 27.5

05 27.5

05 27.5

05 27.4

05 27.2

05 27.2

05 26.8

05 26.8

05 26.7

05 26.5

05 26.5

05 26.5

05 26.5

05 26.1

05 25.9

05 25.9

05 25.9

05 25.9

05 25.8

05 25.5

05 25.4

05 25.4

05 22.7

05 22.7

05 22.6

05 22.5

05 21.9

05 21.8

05 21.4

05 21.3

05 21.0

05 20.8

05 20.5

05 20.2

69 58

69 06

68 57

71 55

70 46

67 26

68 49

63 46

69 51

69 49

69 04

68 47

68 47

67 29

66 36

46 44

08 08

þ46 33

69 56

66 15

68 48

þ20 10

70 10

þ33 24

67 12

11 30

72 30

65 48

69 55

35 44

65 30

69 29

69 30

þ39 21

OC

OCþDN

OCþDN

OC

GC

OCþDN

DN

GX

OC

OC

OC

OCþDN

OCþDN

OCþDN

OC

GX

DN

OC

OC

OCþDN

OC

OC/NE

OCþDN

OCþDN

OC

GX

OC

OCþDN

OC

OC/NE

OCþDN

OC

OC

OC

11.1

10.0

9.9

11.9

12.1p

9.0

8.5p

10.8

11.9

12.5

10.8

8.0p

11.5

9.0

10.6

12.4

–

12.0

12.2

11.6

11.9

–

12.0p

7.5

11.9

12.1

11.8

–

11.8

–

11.2

11.0

11.8

7.0

0

in LMC

0

0

in LMC in LMC in LMC

0

in LMC in LMC

0.80 0

in LMC in LMC in LMC

–

in LMC 0.70

–

1.7

0

in LMC

1.70

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32 in LMC

1.10

13.0

27, 30, 32 0

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

21, 27

14

3, 7

27, 30, 32

27, 30, 32

27, 30, 32

7, 14

27, 30, 32

7

27, 30, 32

14, 21

27, 30, 32

27, 30, 32

27, 30, 32

21

27, 30, 32

27, 30, 32

27, 30, 32

7

3.00  2.60 in LMC

in LMC

0.40 0.8

in LMC

–

0.5

1.9

1.80

Witch Head Nebula

in LMC

in LMC

0

1.90  1.20

180.0  60.0

5.00

0.5

–

–

–

–

in LMC

in LMC

1.00 25.00

h 352 ¼ h 2806

in LMC

in LMC

3.00  0.80

3.3

0

11.00

0.6

0

5.00

0.9

0

in LMC

in LMC

0.7 0.50

h 350

0

10.00

124 2011 2014 1954 2020 2025

h 2899

h 2900

H III-590

h 2903

h 2909

2037 2027 1981

h 593

h 2908

h 362

2038

2015

h 2901

h 2920

2019

h 2905

2033

2016

h 2902

h 579

1931

H I-261 *

1952/M 1

2006

h 2895

1979

2009

h 2897

H III-240

2003

h 2891

h 357

2010

h 2898

2031

2018

h 2904

2021

2004

h 2893

h 2915

2002

h 2890

h 2906

COL

2001

h 2888

1963

1978

h 2878

1964

1994

h 2887

h 2861

1907

H VII-39 *

H IV-21 *

MEN

1974

h 2877 ¼ h 2884

ORI

DOR

DOR

MEN

DOR

TAU

LEP

MEN

DOR

LEP

DOR

LEP

DOR

DOR

DOR

MEN

MEN

AUR

DOR

DOR

DOR

MEN

MEN

DOR

DOR

DOR

DOR

DOR

AUR

DOR

ORI

1924

H III-447

Con

NGC/M

Herschel

05 35.2

05 35.1

05 34.7

05 34.5

05 34.5

05 34.5

05 33.8

05 33.7

05 33.4

05 33.4

05 33.3

05 33.1

05 33.1

05 32.8

05 32.2

05 32.1

05 31.9

05 31.7

05 31.5

05 31.4

05 31.2

05 30.8

05 30.7

05 30.6

05 30.6

05 30.6

05 30.2

05 29.1

05 28.6

05 28.2

05 28.0

05 27.9

05 27.9

04 26

66 55

69 45

70 33

69 44

þ22 01

23 19

70 59

67 26

21 57

36 25

71 44

67 42

14 04

67 40

67 31

69 13

70 10

69 56

þ34 15

66 57

69 09

66 27

70 49

71 04

67 17

66 52

68 44

66 14

69 07

þ35 19

67 24

05 19

RA (2000.0) Dec

OC

OCþDN

OCþDN

OC

OCþDN

SR

GX

OC

OCþDN

GX

GX

OC

DN

GX

OCþDN

OCþDN

OCþDN

GC

OC

OCþDN

OC

OC

OC

OC

OCþDN

OC

OC

OCþDN

GC

OC

OC

OCþDN

GX

Type

4.2

11.9

10.3

11.9

11.6

8.4

11.8

10.8

12.1

10.8

–

10.9

–

11.8

9.0

10.6

–

10.9

10.4

10.1

11.5

11.0

11.3

11.7

10.9

9.6

10.1

–

10.7

9.8

8.2

9.0

12.5

Mag

in LMC in LMC in LMC in LMC in LMC in LMC in LMC in LMC in LMC in LMC

0.60 3.90 0

2.00 2.70 0

2.20 0

0.80 0

in LMC in LMC in LMC in LMC in LMC

0.30 1.00 0

1.00 0

in LMC

1.90

in LMC in LMC

3.40

in LMC in LMC in LMC

1.70 0

0.70 28.0

0

in LMC

0.50 0.5

Crab Nebula

6.00  4.00

1.8

0

0.9

0

5.60  1.80

14.0

in LMC

2.00 0

h 2853

4.20  2.00

1.8

5.6

h 355

6.00

1.0

2.1

2.8

1.7

h 354

Name/Notes

5.00

1.7

0

1.60  1.20

Size

14

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

7

21

27, 30, 32

27, 30, 32

21

21, 22

27, 30, 32

27, 30, 32

14, 21

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

7, 8

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

7

27, 30, 32

14

Map no.

125

2017 2077 2088 2093 2023

h 2896

h 2947

h 2955

h 2963

H IV-24

1961

2074

h 2942

H III-747 *

2070

h 2941

2100

2075

h 2943

h 2966

1996

H VIII-42

2082

2065

h 2938

2024

2053

h 2927

H V-28 *

2055

h 2945

2057

h 2919

h 2931

2041

h 2051

h 2935

2051

H V-34

2058

1990

h 358

h 2933

1960/M 36

h 608

2056

2044

h 2922

h 2932

2042

H III-1

1999

1982/M 43

H III-269

2050

1993

H V-30

H IV-33 *

1977

H V-31 *

h 2928

1976/M 42 1980

h 360

2035

h 2916

CAM

DOR

ORI

DOR

ORI

DOR

DOR

DOR

LEP

DOR

DOR

MEN

TAU

MEN

DOR

DOR

MEN

MEN

MEN

DOR

ORI

DOR

MEN

ORI

AUR

DOR

DOR

ORI

LEP

ORI

ORI

ORI

DOR

05 42.1

05 42.0

05 41.9

05 41.8

05 41.6

05 41.5

05 40.8

05 39.6

05 39.4

05 38.9

05 38.6

05 38.2

05 38.2

05 37.3

05 37.3

05 37.0

05 36.7

05 36.6

05 36.5

05 36.5

05 36.5

05 36.4

05 36.2

05 36.2

05 36.1

05 35.9

05 35.8

05 35.6

05 35.5

05 35.5

05 35.4

05 35.4

05 35.3

þ69 23

69 14

01 51

64 18

02 14

68 55

69 28

69 40

17 51

69 29

69 05

70 40

þ25 49

70 13

67 24

69 24

70 15

70 08

70 40

69 22

06 42

66 58

71 00

01 12

þ34 08

69 11

68 54

05 16

17 49

04 52

05 54

05 27

67 34

GX

OC

DN

GX

DN

OCþDN

OC

OCþDN

OC/NE

OCþDN

DNþOC

OCþDN

OC/NE

OC

OC

OCþDN

OC

OC

OC

OCþDN

DN

OC

OC

DN

OC

OCþDN

OCþDN

DN

GX

DN

DN

DN

OCþDN

10.9

9.6

–

11.8

–

11.6

12.5

–

8.0

8.5p

8.2

11.5

–

11.2

12.2

8.4

12.2

11.9

12.3

9.3

–

10.4

11.7

–

6.0

10.6

9.6

9.0p

12.4

–

–

4.0

– 0

in LMC

0

in LMC in LMC in LMC in LMC

0

0.60 0

2.60

0

in LMC 0

in LMC

in LMC

2.80 4.50  3.10

Flame/Burning Bush Nebula Zeta ORI in field

30.00

1.3  1.2

0

10.00

1.7

1.70

in LMC

¼ multiple star jh 3780 0

150

4.0

–

1, 3

27, 30, 32

14

27, 30, 32

14

27, 30, 32

27, 30, 32

27, 30, 32

14, 21

27, 30, 32

27, 30, 32

27, 30, 32 30.0  20.0

7 2.00

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

14

27, 30, 32

–

1.2

Tarantula Nebula

in LMC

1.80

0

in LMC

1.70 1.8

in LMC

1.00

0

in LMC

0.70 16.0

in LMC

1.70 0

14 27, 30, 32

7, 8 Epsilon ORI Nebula, h 363

50.00  10.00

27, 30, 32

27, 30, 32

14

10.00

2.0

in LMC

part of Orion Nebula

9.00

20.0  15.0

0

14, 21

14

14

27, 30, 32

14

surrounds Iota ORI, h 361

Orion Nebula

in LMC

1.50  1.40 0

0

20.00

14.00

65.0  60.0

3.00

126 2098 2107 2061 2105 2109 2113 2114 2073 2068/M 78 2063 2090 2071 2118 2089 2121 2122 2134 2106 2127 2133 2130 2099/M 37 2136 2135 2112 2140 2145 2157

h 2971

h 2924

h 2969

h 2972

h 2975

h 2974

H III-241

h 368

H VIII-2

h 2944

H IV-36

h 2979

H III-270

h 2982

h 2981

h 2991

h 2967

h 2986

h 2989

h 2987

h 369

h 2992

h 2990

H VII-24

h 2995

h 2998

h 3006

2102

h 730 2026

2096

h 725

H VIII-28

2022

H IV-34 *

h 2965

NGC/M

Herschel

DOR

MEN

DOR

ORI

DOR

DOR

AUR

DOR

MEN

DOR

LEP

MEN

MEN

MEN

LEP

DOR

ORI

COL

ORI

ORI

LEP

DOR

DOR

DOR

DOR

COL

MEN

TAU

DOR

DOR

DOR

ORI

Con

05 57.3

05 54.5

05 54.0

05 53.9

05 53.1

05 52.8

05 52.4

05 52.1

05 51.1

05 51.1

05 50.7

05 50.1

05 48.7

05 48.0

05 47.8

05 47.2

05 47.2

05 47.0

05 46.8

05 46.7

05 45.9

05 45.8

05 45.5

05 44.4

05 44.2

05 43.9

05 43.2

05 43.1

05 42.5

05 42.2

05 42.2

05 42.1

69 11

70 55

68 36

þ00 24

67 26

69 30

þ32 33

67 20

71 11

69 22

21 35

71 07

70 04

71 28

17 36

69 09

þ00 18

34 14

þ08 48

þ00 03

21 59

68 03

69 45

68 32

66 25

33 57

70 37

þ20 07

68 16

69 29

68 28

þ09 05

RA (2000.0) Dec

OC

OC

OC

OC

OC

OC

OC

OC

GC

OC

GX

OC

OCþDN

GC

GX

OC

DN

GX

OC/NE

DN

GX

OC

OCþDN

OCþDN

OC

OC/NE

OC

OC/NE

OCþDN

OC

OC

PN

Type

10.2

12.1

12.4

9.1

12.1

10.5

5.6

12.0

12.0

11.6

12.1

11.1

10.4

12.4

11.0

12.0

8.0p

11.3

–

8.0

12.4

12.5

12.3

12.2

12.2

–

11.5

–

10.7

11.4

11.3

11.6

Mag in LMC in LMC in LMC

0

in LMC

27, 30, 32 in SMC

27, 30, 32

in LMC in SMC in LMC

0

in SMC in LMC

0

2.70

1.7

in LMC

18.0 1.70

h 371

in LMC 0

in LMC 1.00

1.9

0

15.00

1.2

1.2

1.70

27, 30, 32

27, 30, 32

27, 30, 32

14

27, 30, 32

27, 30, 32

7, 8

27, 30, 32

27, 30, 32

27, 30, 32

21, 22

2.70  1.40 0

27, 30, 32

2.50

2.7

4.50

14, 21 0

1.90  1.20

1.3

27, 30, 32

14

7.00  5.00 0

21, 22

4.90  2.40

14 7, 14

–

8.00  6.00

21

27, 30, 32

1.50  1.40

h 2934

0

1.0

27, 30, 32

1.80 in LMC

in LMC

2.00

27, 30, 32

21, 22 27, 30, 32

in LMC

1.70

27, 30, 32

7, 14

27, 30, 32

27, 30, 32

27, 30, 32

7, 14

Map no.

8.00

2.1

0

10.00

1.6

1.2 1.00

Name/Notes

0

0.60

Size

127

2158 2170

H VI-17 *

H IV-19

2204 2206 2207 2202

H VII-13 *

h 3033

h 3032

h 385

ORI

2194

2214

h 3039 2192

2196

H II-265

H VI-5 *

2186

H VII-25 *

H VII-57

DOR

2210

h 3036

ORI

CMA

CMA

CMA

AUR

LEP

ORI

DOR

MON

2213 2185

h 3038

H IV-20 *

MON

GEM

CAR

ORI

LEP

MON

GEM

MON

MEN

2167

H IV-44

MEN

DOR

ORI

2203

h 3035

2180

2187

h 3025

ORI

AUR

H VIII-6

2143

h 374

2182

2126

H VIII-68 *

LEP

GEM

H IV-38

2139

H II-264

2168/M 35

2129

H VIII-26 *

DOR

DOR

h 377

2172

h 3015

2191

2164

h 3011

MEN

DOR

h 3023

2173

h 3018

2179

2160

h 3008

DOR

DOR

2169

2159

h 3007

H VIII-24 *

2156

h 3005

DOR

h 3014

2154

h 3003

06 16.9

06 16.4

06 16.0

06 15.7

06 15.2

06 13.8

06 12.8

06 12.2

06 12.2

06 11.5

06 11.1

06 10.7

06 09.6

06 09.5

06 08.9

06 08.4

06 08.4

06 08.0

06 07.5

06 07.5

06 06.9

06 04.7

06 03.9

06 03.0

06 03.0

06 01.1

06 01.0

05 59.9

05 58.7

05 58.1

05 58.0

05 57.9

05 57.6

05 57.5

þ05 59

21 22

26 46

18 39

þ39 51

þ12 48

68 16

21 48

þ05 27

69 08

06 13

71 33

þ04 43

06 20

þ24 20

52 31

þ13 57

21 45

06 24

þ24 06

06 12

75 26

69 34

þ05 43

þ49 54

23 40

þ23 18

68 38

68 31

72 59

68 17

68 38

68 27

67 15

OC/NE

GX

GX

OC

OC

OC

OC

GX

OC

GC

DN

OC

OC/NE

DN

OC

GX

OC

GX

DN

OC

OCþDN

OC

GX

OC/NE

OC

GX

OC

OC

OC

GC

OC

OC

OC

GC

–

11.0

12.1

8.6

10.9

8.5

10.9

10.9

8.7

10.2

–

12.4

–

–

5.1

11.4

5.9

12.3

–

8.6

6.6p

12.0

12.3

–

10.2

11.6

6.7

11.8

10.3

11.9

12.2

11.4

11.4

11.8 in LMC in LMC in LMC in LMC in LMC

0.90 0

2.40 0

1.70

h 380

6.00

h 3024 in LMC

2.80  2.20 3.60 9.0

21, 22 7.00

3.9  2.2

0

14

22

14, 22

10.0

2.40  1.3

7, 8

8, 14

27, 30

22

14

27, 30

14

27, 30

14

0

5.00

¼ O. Struve 885

h 384

5.00

0

in LMC

2.10

0

h 383

3.00

2.1

0

h 381

2.00

14

27 7, 8

Lassell’s Delight

25.00

8, 14

21, 22

14

7, 8

14

27, 30

27, 30, 32

14

3

21, 22

7, 8

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

27, 30, 32

1.70  0.90

6.00

1.1  0.9

0

“37” Cluster, h 379

in field with open cluster M35, h 375

2.00

tiny nebulous group

5.00

0

0

–

3.30

1.3  0.9

0

11.00

6.0

0

2.40  1.90

6.0

0

2.5

1.2

h 372

in LMC

0

1.1

in LMC

2.40

128 2254 2262 2263 2259 2261

2267 2264 2265

H VII-37

h 3058

H VI-28

H IV-2

h 3059

H VIII-5 ¼ H V-27 *

h 402

H VIII-50 2260

2252

H VIII-3 *

H VIII-48

2251

H VIII-49

H VII-22

2250 2240

h 394

2245

2243

h 3053

H IV-3

2236

H VII-5 2239

2234

H VIII-9

2244

2224

H VII-35

H VII-2 *

2225

H VII-26

h 392

2249 2232

2223

h 3043

H VIII-25 *

2219

h 387

h 3055

2217 2220

h 3041

2215

H VII-20 *

h 3042

NGC/M

Herschel

GEM

MON

CMA

MON

MON

CMA

MON

MON

MON

MON

MON

AUR

MON

MON

MON

MON

CMA

MON

GEM

GEM

MON

MON

DOR

CMA

MON

PUP

CMA

MON

Con

06 41.5

06 41.1

06 40.8

06 39.2

06 38.6

06 38.4

06 38.4

06 38.1

06 36.0

06 35.0

06 34.7

06 32.9

06 32.8

06 32.7

06 32.4

06 31.0

06 29.8

06 29.7

06 29.3

06 27.6

06 26.6

06 26.6

06 25.9

06 24.6

06 23.4

06 21.8

06 21.7

06 21.0

þ11 56

þ09 53

32 29

þ08 44

þ10 53

24 49

þ01 11

01 28

þ07 40

þ05 23

þ08 22

þ35 12

05 02

þ10 10

þ04 52

þ04 57

31 17

þ06 50

þ16 41

þ12 38

09 39

04 45

68 48

22 50

04 41

44 46

27 14

07 17

RA (2000.0) Dec

OC/NE

OCþDN

GX

DN

OC

GX

OC

OC/NE

OC

OC

OC

OC/NE

OC

DN

OC

DN

OC

OC

OC/NE

OC/DN/ NE

OC

OC

GC

GX

OC

OC

GX

OC

Type

–

4.1

12.2

–

10.8

12.1

11.3

–

9.1

7.7p

7.3

–

8.9

–

4.8

4.8

9.4

8.5

–

–

–

4.2

12.2

11.5

–

–

10.7

8.4

Mag

0

6.0

10.00

40.0

0

1.70  1.30

3.00  1.00

3.5

0

2.60  2.00

4.0

0

20.00

Christmas Tree Cluster þ Cone Nebula, h 401

Hubble’s Variable Nebula, surrounds R MON, h 399

h 400

h 398

h 397

8, 14

8, 14

22

14

8, 14

22

14

14

14

14

h 396

20.00 0

14

h 395

10.00

14

8, 14

14

14

8

10.0

Rosette Cluster, surrounds 12 MON

Rosette Nebula

22

–

0

5.00  4.00

24.00

24.0

8.30

14

h 390

0

8.0

8, 14

h 389

5.00

14, 22 8, 14

h 388

40.00

27, 30 14

–

surrounds 10 MON

45.00

1.7 in LMC

22

0

14

3.00  2.60

21, 22, 27

22

24

Map no.

10.00

5.00

4.7  4.3 small asterism

h 386 0

8.00 0

Name/Notes

Size

129

2319 2328 2325 2348

H VIII-1

h 3072

h 3071

h 3074

2327

2316

H II-304

H IV-25

2318

H VII-14

2323/M 50

2312

h 419

2324

2311

H VIII-60 *

H VII-38 *

2309

H VI-18

h 425

2304

H VI-2 *

PUP

2310 2306

h 3069

H VIII-39

H VIII-51

MON

2301 2302

H VI-27 *

PUP

CMA

MON

MON

VOL

CMA

PUP

MON

MON

CMA

MON

MON

MON

GEM

MON

MON

AUR

2298 2281

VOL

H VIII-71 *

2307

h 3068

VOL

CMA

MON

GEM

CMA

CMA

CMA

MON

MON

GEM

CMA

CMA

CAM

h 3065

2305

h 3067

2287/M 41

h 411

2292/2293

2283

H III-271

h 3063

2280

h 3062

2274

2270

H VII-36

2286

2269

H VI-3

H VIII-31 *

2266

H VI-21 *

H II-615

2272 2271

h 3061

h 3060

2253

H VII-54

07 04.3

07 04.2

07 03.2

07 03.1

07 02.7

07 02.5

07 01.1

06 59.7

06 59.5

06 58.8

06 57.8

06 56.2

06 55.0

06 54.6

06 54.0

06 51.9

06 51.8

06 49.3

06 49.0

06 48.8

06 48.6

06 47.6

06 47.6

06 47.2

06 46.0

06 45.9

06 44.8

06 43.9

06 43.9

06 43.2

06 42.8

06 42.7

06 42.4

11 18

þ01 03

08 20

67 23

28 42

42 03

þ03 04

07 46

13 42

þ10 16

04 35

07 12

þ18 01

07 11

40 52

07 04

þ00 28

þ41 04

36 00

64 20

64 16

26 45

03 10

þ33 34

20 44

18 14

27 38

þ03 26

þ04 34

þ26 58

23 28

27 27

þ66 20

DN

OC

OC

OC/NE

GX

GX

OC/NE

DN

OC

OC/NE

OC

OC

OC

OC/NE

GX

OC

OC

OC

GC

GX

GX

GX

OC

GX

OC

GX

GX

OC/NE

OC

OC

GX

GX

OC/NE

–

8.4

5.9

–

11.0

11.8

–

–

–

–

9.6

10.5

10.0

–

11.7

8.9

6.0

5.4

9.3

12.3

118

10.8/ 11.2

7.5

12.4

4.5

12.2

10.5

–

10.0

9.5

12.0

11.8

–

h 404

–

0

0

0

h 417 h 418

5.00 0

h 428

1.00

14, 15, 22

14, 15

14, 15 h 427

8.00

15.0

27, 30

22

22, 27

14, 15

0

0

h 423

14, 15

14, 22

8, 14

14

14

8, 14

14

22, 27

14

14

3, 8

11.00

3.0  1.5

0

1.30  0.80

–

4.00  3.00

–

5.00  2.50 h 3070

h 415

3.00 7.0

h 416

0

h 414

h 413

–

4.3  0.8

0

2.50

15.0

0

25.00

5.0

22

27, 30

0

27, 30

22

14

8

1.70  1.60

galaxy pair

h 408

h 406

22

14, 22

22

14

14

2.10  1.50

4.0  3.5 / 4.00  3.20

0

15.00

1.2  1.1

0

39.00

3.6  2.7

0

6.30  3.00

h 405

h 403

5.0 3.00

8

22

0

2.4  1.6 22

1, 3

2.10  1.40

0

0

–

130 2360 2359 2362 2381 2367

H VII-12 *

H V-21

H VII-17 *

h 3084

H VIII-27

2380¼2382 2374 2383 2384 2371/2372 2395

h 3079 ¼ h 3082

H VIII-35

h 3081

h 3083

H II-316/H II 317 *

H VIII-11 *

2368

2355 ¼ 2356

H VI-6 * ¼ H VII-6

2397

2358

H VIII-45

h 3085

2369

h 3078

h 443

2347

H III-746

2352

H VII-15 2354

2340

H II-736

2353

2349

H VII-27

H VIII-34 *

2346

H IV-65

H VII-16 *

2345 2329

2343

H VIII-33 *

H III-875 ¼ H II 735

2339

H II-769

h 3073

2335 2331

H VIII-32 *

2320

H II-861

H VIII-40

NGC/M

Herschel

GEM

GEM

CMA

CMA

CMA

CMA

VOL

MON

CMA

CAR

CMA

CMA

CMA

GEM

CMA

CAR

CAM

MON

CMA

CMA

LYN

MON

MON

LYN

CMA

MON

GEM

GEM

MON

LYN

Con

07 27.1

07 25.6

07 25.1

07 24.8

07 24.0

07 23.9

07 21.3

07 21.0

07 20.1

07 20.0

07 18.8

07 18.6

07 17.8

07 16.9

07 16.8

07 16.6

07 16.1

07 14.6

07 14.3

07 13.6

07 11.0

07 10.0

07 09.4

07 09.2

07 08.3

07 08.3

07 08.3

07 07.2

07 06.6

07 05.6

þ13 35

þ29 29

21 02

20 56

13 16

27 31

69 00

10 23

21 56

63 04

24 57

13 12

15 37

þ13 47

17 03

62 21

þ64 43

10 18

25 44

24 06

þ50 10

08 37

00 48

þ48 37

13 10

10 39

þ18 47

þ27 21

10 05

þ50 36

RA (2000.0) Dec

OC

PN

OC

OC

OC

GX

GX

OC

OC

GX

OC

DN

OC

OC

OC/NE

GX

GX

OC

OC

OC/NE

GX

OC/NE

PN

GX

OC

OC

GX

OC

OC

GX

Type

8.0

11.2

7.4

8.4

8.0

11.3

11.9

11.8

7.9

12.5

3.8

–

7.2

9.7

–

12.3

12.4

7.1

6.5

–

11.9

–

11.6

12.5

7.7

6.7

11.7

8.5

7.2

12.1

Mag h 424

1.40  0.80

0

15.00

1.0

Peanut Nebula, h 445/ h 445

8, 14, 15

8

22 0

22

14, 15, 22

22

27, 30

5.00

0

14, 15

5.00

12.00

2.1  2.0

0

2.50  1.20

3.0

0

h 3080

22

22

Tau CMA Cluster, h 441 ¼ h 3077

6.00

14, 15, 22 14, 15, 22

27, 28, 30

Thor’s Helmet/Duck Nebula, 3075

9.00  6.00

5.00

CH 2, h 440 ¼ h 3076

14.00

8, 14, 15

14, 15, 22

27, 28, 30

1, 3, 4

14, 15, 22

22

22

3, 8

14, 15

14, 15

3, 8

14, 15, 22

14, 15, 22

8, 14, 15

8

14, 15, 22

3, 8

Map no.

1.40

h 439

h 438

8.00

8.0

0

3.50  1.10

1.8  1.3

0

18.00

18.0

0

h 433

1.80  1.20 5.00

CH 4, h 436

h 429

–

0.90

1.30  1.10

12.0

0

h 434

2.70  2.00 6.00

h 432

19.00

7.0

0

Name/Notes

Size

131

2423 2419 2425

H VII-28 *

H I-218 *

H VIII-87

2439 2432 2438 2437/M 46 2440 2447/M 93 2448 2451 2452

h 3094

H VI-36

H IV-39 *

h 463

H IV-64 *

h 3098

h 466

h 3099

h 3100

2408

2415

H II-821

2430

2403

H V-44 *

h 452

2422/M 47

H VIII-38 *

H VIII-46

2442

h 3097

2420

2421

H VII-67 *

2428

2434

h 3096

H VIII-47

2414

H VIII-37

H VI-1 *

2413

H VIII-52

2401

H VII-65 2417

2392

H IV 45 *

2409

2366

H III-748

h 3087

2394

H VIII-44

h 3086

2396

H VIII-36

PUP

PUP

PUP

PUP

PUP

PUP

PUP

PUP

PUP

CAM

PUP

PUP

GEM

PUP

LYN

PUP

LYN

CAM

PUP

VOL

PUP

VOL

PUP

PUP

PUP

CAR

PUP

GEM

CAM

CMI

PUP

07 47.4

07 45.4

07 44.6

07 44.6

07 41.9

07 41.8

07 41.8

07 40.9

07 40.8

07 40.5

07 39.4

07 39.2

07 38.5

07 38.3

07 38.1

07 37.1

07 36.9

07 36.9

07 36.6

07 36.4

07 36.3

07 34.9

07 33.3

07 33.3

07 31.6

07 30.1

07 29.4

07 29.2

07 28.9

07 28.6

07 28.1

27 20

37 58

24 41

23 52

18 13

14 49

14 44

19 05

31 39

þ71 39

16 21

16 31

þ21 34

14 52

þ38 53

13 52

þ35 15

þ65 36

14 30

69 32

20 37

69 17

15 27

13 06

17 11

62 15

13 58

þ20 55

þ69 13

þ07 02

11 44

PN

OC

OC/NE

OC

PN

OC

PN

OC

OC

OC

OC/NE

OC/NE

OC

OC

GC

OC

GX

GX

OC

GX

OC

GX

OC

OC/NE

OC/NE

GX

OC

PN

GX

OC/NE

OC

12.0

2.8

–

6.2

9.4

6.1

10.8

10.2

6.9

–

–

–

8.3

–

10.3

6.7

12.2

8.2

4.4

10.4

8.3

11.3

7.9

–

7.3

12.1

12.6

9.1

10.9

–

7.4

14, 15, 22 22

14, 15, 22

0.50

22

22, 27

CH 1

10.00

surrounding c PUP

h 3095

1.30

50.00

CH 3

20.00

14, 15, 22

22

in open cluster M 46, h 464 ¼ h 3039

1.30

14, 15, 22

5.00

h 3092

9.0

7.00

22

1, 3 0

14, 15, 22

14, 15, 22

8

14, 15, 22

3, 8

14, 15, 22

8

10.00

h 458

Intergalactic Wanderer, h 457

h 3090

h 456

1, 3, 4

–

13.00

6.0

0

5.00

4.6

0

12.00

0.9

0

h 459 ¼ h 3088

14, 15, 22

23.40  11.80

25.0

27, 28, 30

22

0

h 3089

27, 28, 30

6.00  5.00

8.0

0

2.40  2.20

14, 15, 22

14, 15, 22

27, 28, 30

14, 15, 22

14, 15, 22 h 455

h 454

6.00

0

8

–

2.50

2.8  1.9

0

2.00

0.9 Eskimo/Clown Face Nebula, h 450

1, 3, 4

0

14, 15

14, 15, 22

–

h 451

8.10  3.00

10.00

132 2516 2506 2493 2509 2500 2513 2517 2527 ¼ 2520 2525

h 3111

H VI-37 *

H III-750

H VIII-1 *

H III-709

H III-512

h 3110

H VIII-30 *

H III-877

2555 2564 2567

H III-256

h 3119

H VII-64 *

PUP

2559

2541

H III-710 2554

2545

H II-627

h 3118

2548/M 48

H VI-22 *

H II-303

LYN

2537

H IV-55

PUP

PUP

PUP

HYD

CNC

CNC

HYD

LYN

LYN

2546 2543

H II-719

VEL

PUP

LYN

PUP

PUP

CNC

LYN

PUP

LYN

MON

CAR

PUP

CAR

PUP

PUP

PUP

PUP

PUP

PUP

h 3116

2547

2489

H VII-23 *

h 3117

2502

h 3109

2539

2483

h 3105

H VII-11 *

PUP

2479

H VII-58 *

2533

2482

H VII-10 *

2532

2467

H IV-22

h 3113

2477

h 3103

H II-726

PUP

2455

h 3102

PUP

2453

h 3101

Con

NGC/M

Herschel

08 18.6

08 18.6

08 18.0

08 17.9

08 17.1

08 14.7

08 14.2

08 13.8

08 13.2

08 13.0

08 12.4

08 10.7

08 10.7

08 10.2

08 07.0

08 05.6

08 05.3

08 02.8

08 02.5

08 01.9

08 00.7

08 00.4

08 00.2

07 58.3

07 56.2

07 55.9

07 55.9

07 55.1

07 54.9

07 52.6

07 52.3

07 49.0

07 47.8

30 38

21 49

þ00 44

þ23 28

27 28

þ49 04

þ21 21

05 48

þ46 00

þ36 15

37 38

49 16

12 50

þ33 57

29 54

11 26

28 10

12 19

þ09 25

þ50 44

19 04

þ39 50

10 47

60 52

30 04

52 18

27 56

17 43

24 18

26 23

38 33

21 18

27 14

RA (2000.0) Dec

OC

GX

GX

GX

GX

GX

GX

OC

GX

GX

OC

OC

OC

GX

OC

GX

OC

GX

GX

GX

OC

GX

OC

OC

OC

GX

OC

OC

OC

OCþDN

OC

OC

OC

Type

7.4

12.5

12.5

12.0

10.9

11.5

12.4

5.8

11.7

11.9

6.3

4.7

6.5

12.3

7.6

11.6

6.5

11.8

11.6

11.5

9.3

12.0

7.6

3.8

7.9

12.2

7.6

9.6

7.3

7.1

5.8

10.2

8.3

Mag 0

15.0

12.0

h 483

2.50  2.00

h 488 h 486

3.00  2.00

h 492

h 503 ¼ h 3120

22

11.0

22

15 0

h 498

1.90  1.40

8

22

3, 8

8

15

3, 8

1.20  0.80

h 497

3.20  2.40

3.0  1.4

0

0

h 494 6.30  3.20

2.2  1.2

0

CH 5, h 496

30.00 0

Bear Paw Galaxy, h 491

1.70  1.50

3, 8

22, 27 h 493

2.30  1.20

70.0

22, 27

15, 22 0

h 3114

15.00

3, 8

22

15, 22

22

15, 22

15

3, 8

14, 15, 22

3, 8

14, 15

27, 28, 30

25.00

h 489

1.90  1.40

6.0

0

10.0

0

1.40  1.00

h 478

0

h 476

h 480

2.90  2.70

12.0

1.90

0

22.00

5.0

22

27 h 479 ¼ h 3107

22

2.10  1.30 0

15, 15, 22

22

22

22, 27

22

22

Map no.

9.00

h 474 ¼ h 3106

h 472

Name/Notes

11.00

10.00

0

20.00

15.0

4.00

Size

133

2639 2649 2669

H I-204

H II-727

h 3140

2664

2658

h 4017

2629

2648

H III-49

h 524

2659

h 3137

H III-982

2660

h 3138

2671

2632/M 44

h 517

2670

2645

h 3136

h 3141

2635

h 3133

h 3142

2640

2608

H II-318

h 3134

VEL

2613

H II-266 * 2626

2610

H IV-35

2627

2599

H III-234

h 3131

2609

h 3130

H VII-63 *

CNC

2595

H III-599

VOL

CNC

UMA

VEL

VEL

VEL

LYN

UMA

PYX

CNC

VEL

VEL

CNC

VEL

PYX

CAR

PYX

PYX

HYD

CNC

CAR

CNC

CNC

2601 2592

PUP

PUP

H II-315

2587

h 3124

CNC

PUP

PUP

CNC

LYN

PUP

PUP

h 3126

2588

h 3125

2579

h 3122 2580

2563

H II-634

2577

2549

h 495

H II-259

2571

H VI-39 *

h 3123

2566

H III-288

08 47.2

08 47.2

08 46.2

08 45.5

08 44.9

08 44.1

08 43.6

08 43.4

08 42.7

08 42.6

08 42.2

08 40.1

08 38.9

08 38.5

08 37.4

08 37.3

08 35.6

08 35.3

08 33.4

08 33.4

08 32.2

08 29.5

08 27.7

08 27.1

08 25.5

08 23.5

08 23.2

08 22.7

08 21.6

08 21.1

08 20.6

08 19.0

08 18.9

08 18.7

þ12 36

þ72 59

41 53

48 47

52 58

þ34 43

þ50 12

32 39

þ14 17

44 57

47 09

þ19 59

46 13

34 46

55 07

29 57

40 40

þ28 28

22 58

16 09

þ22 34

61 06

þ21 29

þ25 58

68 07

29 30

32 59

þ22 33

30 19

36 11

þ21 04

þ57 48

29 44

25 29

OC/NE

GX

OC

OC

OC

GX

GX

OC

GX

OC

OC

OC

OC/NE

OC

GX

OC

DN

GX

GX

PN

GX

OC

GX

GX

GX

OC

OC

GX

OC

OCþDN

GX

GX

OC

GX

–

12.3

11.6

7.8

6.1

12.3

11.7

9.2

12.0

8.6

8.8

3.5

7.0

11.2

11.7

8.4

–

12.2

10.4

12.7

12.2

–

12.3

12.4

12.5

9.2

11.8

12.5

9.7

7.5

12.3

11.2

7.0

11.0

0

h 512

1.90  1.20 5.0

h 522 7.0

5.00

1.5  1.3

0

5.00

0

14.00

0

h 518 1.50  1.40

1.8  1.1

0

0

10.00

3.2  1.1

h 521 ¼ h 3135

8, 15

1, 3, 4

22

22, 27, 28

27, 28

8

3, 4, 8

22

8, 15

22, 27 0

22, 27 15.00 0

22, 27 8, 15 3.00

70.00

3.0

Beehive Cluster

22 0

27, 28 3.00

22

22, 27

8

22

15, 22

8

27, 28, 30

8

8

27, 28, 30

22

22

8

22

22, 27

8

1, 3, 4

22

22

2.20  1.90

9.00

h 516 ¼ h 3132

h 3129

6.50  1.40 0

h 513 ¼ h 3127

h 507

0.70

1.9  1.7

0

0

h 506

3.20  2.40 6.00

h 505

0

h 501

h 502

1.70  1.40

1.6  1.1

0

10.00

2.0

0

1.80  1.10

8.0

0

19.00

2.0  1.7

0

3.80  1.20

7.0

0

2.90  1.70

134 2732 2783 2748

h 548

2792

h 3149

H III-295

2784

H I-59

h 539

2776

2808

h 3152 2778

2768

H I-250 *

H II-564

2781

H I-66

h 563

2775

H I-2 *

2726

H II-834

2770

2736

h 3145

2756

2712

h 540

H II-490

2701

H IV-66

H II-828

2721

H II-529

2765

2718

H II-557

H II-520

2717

h 3144

2742

2693

H II-823

H I-249 *

2708

H II-281

2750

2655

H I-288 *

2763

2695

H II-280

H III-291

2681

H I-242 *

H III-275

2682/M 67 2683

2678

H VIII-10

h 531

2672

H II-48

H I-200 *

NGC/M

Herschel

CAM

CNC

CAM

VEL

HYD

LYN

LYN

CAR

UMA

HYD

CNC

LYN

UMA

HYD

UMA

HYD

CNC

UMA

VEL

LYN

UMA

HYD

HYD

PYX

UMA

HYD

CAM

HYD

UMA

LYN

CNC

CNC

CNC

Con

09 13.7

09 13.6

09 13.4

09 12.4

09 12.3

09 12.3

09 12.2

09 12.0

09 11.6

09 11.5

09 10.3

09 09.6

09 09.0

09 07.6

09 07.6

09 06.8

09 05.7

09 04.9

09 00.4

08 59.5

08 59.1

08 58.9

08 58.9

08 57.0

08 57.0

08 56.1

08 55.6

09 54.5

08 53.5

08 52.7

08 50.4

08 50.2

08 49.3

þ76 29

þ29 59

þ79 11

42 26

24 10

þ35 01

þ44 57

64 52

þ60 02

14 49

þ07 02

þ33 07

þ53 51

þ03 23

þ60 29

15 30

þ25 26

þ59 56

45 54

þ44 55

þ53 46

04 46

þ06 18

24 40

þ51 21

03 22

þ78 13

03 05

þ51 19

þ33 25

þ11 49

þ11 20

þ19 04

RA (2000.0) Dec

GX

GX

GX

PN

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

SR

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

OC/NE

GX

Type

11.5

12.2

11.9

11.6

10.3

12.3

11.4

6.2

9.9

11.6

10.4

12.0

12.4

12.2

11.4

12.0

12.0

12.4

–

11.9

12.0

12.2

12.2

12.3

11.7

12.0

10.1

11.9

10.2

9.7

6.9

–

11.6

Mag

0

0

h 571 ¼ h 3148

5.50  2.20

3.1  1.1

1, 3, 4

8 0

0

1

2.1  0.9

2.20  1.50

22

22

8

4, 8, 9

27, 28, 30

3, 4

15, 22

15

8

3, 4

15

3, 4

15, 22

8

3, 4

22, 27, 28

8

3, 4

15

15

22

3, 4

15

1

15

3, 4

8

8, 15

8, 15

8, 15

Map no.

0

0

0.40

h 566

1.40  1.00

2.8  2.5

0

0

h 555

6.40  3.00 14.00

h 569 ¼ h 3147

3.00  1.50

4.3  3.3

0

h 564

h 562 0

h 553

1.7  1.2

3.70  1.10

h 558

2.10  1.10 0

h 550

3.00  1.50 0

h 560

0

h 545

Herschel’s Ray/Pencil

h 537

h 543

h 542

h 535

2.30  2.00

2.2  1.9

0

1.60  0.50

20.0  2.0

0

2.80  1.50

2.6  1.6

0

2.40  1.60

2.1

0

2.10  1.50

2.6  1.8

0

2.70  1.40

4.9  4.1 h 520

h 536

1.70  1.20 0

h 530

3.60  3.30 0

h 532

9.30  2.10

0

h 528

10.00 25.0

h 526

3.00  2.80 0

Name/Notes

Size

135

VEL

2907 2903/2905

H II-506

H I-56/H I-57 *

h 3170 2910

2904

H I-260

2902

2880

H III-8

H III-276

2894

H II-555

h 3171

2899 2889

h 3169

2915

2872

H II-57 ¼ H II-546 2891

2859

H I-137 *

h 3174

2865

h 3161

h 3177

2887

h 3168

VEL

2866 2810

h 3162

2841

H I-205 *

H III-749

UMA

2820

H II-869

LEO

HYD

HYD

VEL

ANT

UMA

LEO

HYD

VEL

PYX

CHA

LEO

LMI

HYD

CAR

UMA

UMA

HYD

CAR

UMA

2867

H III-878

HYD

2855

2805

H III-488

VEL LYN

H I-132

2848

H I-113

UMA

HYD

PYX

CAR

h 3163

2849 2830

h 3160

2845

2815

H III-242 2787

2811

H II-505 *

h 3159

2818

h 3154

H I-216 *

HYD

2842

h 3158

CAR LYN

2822 2782

H I-167 *

CAR

h 3156

2836

h 3157

09 32.2

09 31.6

09 30.9

09 30.4

09 30.2

09 29.6

09 29.4

09 27.2

09 27.0

09 26.8

09 26.2

09 25.7

09 24.3

09 23.5

09 23.3

09 22.1

09 22.0

09 22.0

09 21.8

09 21.5

09 21.4

09 20.3

09 20.2

09 19.7

09 19.3

09 19.3

09 18.6

09 16.3

09 16.2

09 16.0

09 15.6

09 14.1

09 14.0

09 13.7

þ21 30

16 44

14 44

52 54

30 23

þ62 30

þ07 43

11 38

56 06

24 49

76 38

þ11 26

þ34 31

23 10

63 49

þ71 50

51 05

þ50 58

þ64 16

11 55

58 19

þ64 06

16 32

þ33 44

40 31

þ69 12

38 00

23 38

16 19

36 37

63 04

þ40 07

69 38

69 20

GX

GX

GX

OC

GX

GX

GX

GX

PN

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

PN

GX

GX

CX

OC

GX

GX

GX

GX

OCþPN

GX

GX

GX

GX

8.8

11.8

12.2

7.2

12.5

11.5

12.4

11.7

11.8

12.5

12.3

11.9

10.9

11.5

11.7

12.2

–

9.3

12.5

11.7

9.7

10.9

11.8

13.9

12.5

10.8

12.3

12.0

11.4

8.2

12.5

11.4

10.6

11.8 0

0

h 587

2.50  1.50

h 597

h 596

2.00  1.20 6.0

0

12.60  6.00

2.0  1.2

0

1.60  1.30

0

1.20  0.80

h 604

h 607

h 603

1.90  1.00

8

15, 22

15, 22

27, 28

22

3, 4

15

27, 28 15, 22

h 600

2.0  1.0

2.30  1.90

22

28, 30

8, 15

8

0

0

1.50  1.40

1.9  0.9

0

0

h 593 2.10  1.80

4.6  4.1

0

0

22

27, 28 2.50  1.80

2.1  1.6

1, 3, 4 0

27, 28

3, 4

1, 3, 4

15, 22

27, 28

1, 3, 4

15, 22

8

22

1, 3, 4

22

22

15, 22

1.70 0

h 584

8.10  3.50 20.0

h 576

4.10  0.40 0

h 592

2.50  2.20

0.4

0

6.30  4.80

h 582

h 3153

1.20  0.30

3.0

0

3.40  2.00

2.3  1.2

0

3.50  1.10

2.5  0.9

0

22

0

27, 28 h 580 ¼ h 3151

27, 28, 30 8

8.00

h 568

27, 28, 30

1.60  1.30

3.70  2.40

3.3  2.2

0

2.70  2.00

136 2982 2950 2974 2964 2968 2983 2977

h 3184

H IV-68 *

H I-61 *

H I-114 *

H II-491

H III-289

H I-282

2991 3003 2998 3033 3020

H V-26

H II-717

h 3194

H III-51

h 3190 2876

3001

H III-277

H I-285 *

2992

H V-50

h 634

2999 2997

h 3191

2995

2967

H II-275

2986

2960

h 621

H II-311

2954

h 3181

h 3189

2942 2972 ¼ 2999

h 3183 ¼ h 3191

2945

h 3180

h 613

2935

H II-556

HYD

2924 2918

h 3175

2916

H II-260

H III-298

LEO

2921

H III-597

VEL

LEO

VEL

UMA

LMI

UMA

LEO

ANT

HYD

ANT

VEL

HYD

VEL

DRA

HYD

LEO

LEO

SEX

UMA

VEL

SEX

HYD

LEO

VEL

LMI

HYD

HYD

LEO

HYD

LEO

2925 2911

h 3177

H II-40

LEO

2906

H II-495

Con

NGC/M

Herschel

09 50.1

09 48.8

09 48.7

09 48.6

09 47.3

09 46.8

09 46.3

09 45.7

09 45.6

09 45.2

09 44.3

09 44.1

09 43.8

09 43.7

09 43.2

09 42.9

09 42.6

09 42.6

09 42.4

09 42.1

09 40.6

09 40.5

09 40.3

09 39.1

09 37.6

09 36.7

09 35.8

09 35.2

09 35.0

09 34.7

09 33.8

09 33.7

09 32.2

þ12 49

56 25

þ44 05

þ33 25

þ67 55

þ22 01

30 26

14 20

31 11

50 26

21 17

54 47

þ74 52

20 29

þ31 56

þ31 51

03 42

þ58 51

44 12

þ00 20

þ03 34

þ14 55

50 20

þ34 00

22 02

21 08

þ31 42

16 24

þ21 42

20 57

þ10 09

53 26

þ08 27

RA (2000.0) Dec

GX

OC

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

OC/NE

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

Type

12.2

8.8

12.4

11.5

10.1

12.5

11.8

12.2

9.4

9.9

10.7

–

12.5

11.9

11.9

11.2

10.9

10.9

–

11.6

12.5

12.3

9.9

12.5

12.2

11.4

12.5

12.3

11.9

11.9

11.5

8.3

12.5

Mag

h 610

2.50  1.70

0

0

h 616 h 630

h 635

3.70  0.90

3.0  1.6

0

12.00

2.7  1.2

0

h 646 ¼ h 642

h 638

h 639 0

5.70  1.40 0

h 625

0

5.90  2.70

1.4  1.1

0

2.90  2.00

h 3188

8.90  6.80

5.0

0

8, 15

27, 28

4, 8, 9

4, 8, 9

1, 3, 4

8

22, 23

15, 22

22, 23

28

22

27, 28 3.20  2.60

20.0

1, 3, 4 0

22

8, 9

8, 9

15

3, 4

22, 28

15

15

8, 15

28

8, 9

22

22

8, 9

15, 22

8

1.80  0.80

2.5  1.4

0

h 3185

h 624 0

h 622 2.10  1.60

3.0  1.7

0

0

2.7  1.8

3.40  2.10

0

0

0

12.00

3.0  2.8

0

1.40  1.00

1.2  0.9

0

5.00

1.9  1.5

0

h 626

h 3178

3.70  2.80 1.60  1.20

h 611

1.40  1.00

1.3  1.2

0

0

h 3173

2.90  1.10 22

27, 28 8, 15

15.0 h 608

8, 15

4.00  3.10

h 606

1.40  0.90

Map no.

0

Name/Notes

Size

137

3055 3031/M 81 3027 3034/M 82 3070 3067 3078

H VI-4

h 649

H V-23

H IV-79 *

H II-59

H II-492

H II-268

3079 3098 3108 3114 3109 3077 3149

h 663

h 3220

h 3224

h 3221

H I-286 *

h 3234

h 3218

H V-47 *

3100

H II-293

3105

3091

h 3216

3065

3095

h 3214

H II-333

3089

H III-596

h 3219

3087 3081

h 3213

3082

3056

h 3203

3084

3052

H III-272

h 3210

3051

h 3201

h 3211

3044

H III-254

LEO

3032 3041

h 650

H II-98

LMI

3021

H I-115

CHA

UMA

HYD

CAR

ANT

LEO

UMA

UMA

VEL

ANT

HYD

ANT

ANT

HYD

ANT

ANT

ANT

HYD

LEO

LEO

UMA

UMA

UMA

SEX

ANT

HYD

ANT

SEX

LEO

UMA

2985

H I-78 *

CAR

3059

h 3205

10 03.8

10 03.3

10 03.1

10 02.7

10 02.6

10 02.3

10 02.0

10 01.9

10 00.8

10 00.7

10 00.2

10 00.1

09 59.6

09 59.5

09 59.2

09 59.0

09 58.9

09 58.4

09 58.4

09 58.0

09 55.8

09 55.7

09 55.6

09 55.3

09 54.5

09 54.5

09 53.8

09 53.7

09 53.1

09 52.1

09 51.0

09 50.4

09 50.2

80 25

þ68 44

26 09

60 07

31 41

þ24 43

þ55 41

þ72 10

54 46

31 40

19 38

31 33

28 20

22 50

34 13

27 08

30 20

26 56

þ32 22

þ10 22

þ69 41

þ72 12

þ69 04

þ04 16

28 18

18 38

27 17

þ01 35

þ16 41

þ29 14

þ33 33

þ72 17

73 55

GX

GX

GX

OC

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

12.3

10.0

9.8

4.2

11.8

12.1

10.8

11.6

9.7

11.1

11.2

11.6

12.5

12.0

10.8

12.4

12.5

11.1

12.0

12.2

8.6

11.5

7.0

11.9

11.7

12.1

11.8

11.8

11.7

12.5

12.2

10.4

10.8

0

0

h 657

0

22, 23 27, 28

0

0

1.00  1.90

5.2  4.7

0

19.10  3.70

30

1, 3, 4

22, 23

8, 9 2.50  1.80 35.0

3, 4

h 658

27,28 1, 2, 4 2.20  0.60

h 654

22, 23

8.10  1.30

1.70  1.50

2.0

0

3.20  1.70

3.0  1.9

15, 16, 22, 23

22, 23 0

0

22, 23

1.8  1.0

3.60  2.00

22, 23 0

0

2.20  1.80

2.0

h 3215

22, 23 0

22, 23

22, 23

1.8  0.7

1.80  1.60

22, 23

8, 9

15

1, 3, 4

1, 3, 4

1, 3, 4

15

22, 23

15, 22, 23

22, 23

15

8, 15

8, 9

4, 8, 9

1, 3, 4

27, 28, 30

0

0

2.70  2.30

h 3209

h 659

1.40 2.4  0.9

Bode’s Nebula/Cigar Galaxy

11.20  4.30

0

h 643

3.90  1.40

h 656 Bode’s Nebula

0

h 3202

24.90  11.50

2.1  1.3

0

1.80  1.10

2.1  1.3

0

2.10  1.90

4.7  0.7

0

3.70  2.40

1.7  1.3

0

h 652

h 645

0

h 629

1.50  0.90

4.6  3.4

0

0

3.60  3.20

138 3203 3223 3224 3206 3228

h 3243

h 3244

H I-266

h 3245

3182

H I- 265 3198

3193

H II-45 *

H I-199 *

3184

h 3240

3190

H I-168 *

3169

H I-4 *

H II-44 *

3166

H I-3 *

3211

3158

H II-639

3201

3162

H II-43

h 3242

3156

H III-255

h 3238

3145

H III-518

3199

3195

h 3241

h 3239

3137

h 3230

3147

3132

h 3228

H I-79 *

ANT

3124

h 3226

3175

3125

h 3227

3177

3136

h 3229 ¼ h 3231

h 3236

3115

H I-163 *

H III-25

SEX

3106

H II-320

VEL

UMA

ANT

ANT

UMA

HYD

UMA

LEO

UMA

LEO

CAR

VEL

CAR

DRA

LEO

SEX

LMI

LEO

SEX

HYD

CHA

ANT

VEL

HYD

ANT

CAR

SEX

LMI

LMI

3104

H IV-48

Con

NGC/M

Herschel

10 21.8

10 21.8

10 21.6

10 21.6

10 19.9

10 19.6

10 19.5

10 18.4

10 18.4

10 18.1

10 17.8

10 17.6

10 17.1

10 16.9

10 16.6

10 14.7

10 14.2

10 13.8

10 13.8

10 13.5

10 12.7

10 10.2

10 09.5

10 09.2

10 07.0

10 06.7

10 06.6

10 05.8

10 05.2

10 03.9

10 03.9

51 43

þ56 56

34 42

34 16

þ45 33

26 42

þ58 12

þ21 54

þ41 25

þ21 50

62 40

46 25

57 55

þ73 24

þ21 07

28 52

þ30 28

þ03 26

þ38 46

þ22 44

þ03 08

12 26

80 52

29 04

40 26

19 13

29 56

67 23

07 43

þ31 11

þ40 45

RA (2000.0) Dec

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

PN

GC

DN

GX

GX

GX

GX

GX

GX

GX

GX

GX

PN

GX

PN

GX

GX

GX

GX

GX

GC

Type

6.0

11.9

11.3

11.0

10.2

12.2

12.0

10.8

9.6

11.1

10.7

6.9

–

10.6

12.2

11.3

10.3

10.5

11.9

11.4

12.1

11.7

11.6

11.5

9.2

12.0

12.5

10.7

9.1

12.3

13.2

Mag

h 673 h 680 h 682 h 678

2.00  1.80

h 685

h 674

3.90  3.50 20.0

h 689

0

h 697 5.00

2.9  1.9

28

3, 4

22, 23 0

0

22, 23

4.1  2.7

1.90  1.50

4, 8, 9

23

3, 4

9

4, 8, 9

9

27, 28

22, 23, 28

27, 28

1, 4

9

22, 23

15, 16

15, 16

4, 8, 9

9

15, 16

15, 16, 23

0

0

8.50  3.30

2.8  0.6

0

1.80  1.50

2.0

0

h 693

h 692 7.40  6.90

4.4  1.5

0

0

0.30

0

20.00  15.00

h 678

1.50  1.20

5.1  1.3

0

0

h 684

4.20  2.90

4.8  2.3

0

0

3.1  2.7

0

0

3.0  1.6 1.90  0.90

30

0

0

22, 23

0.70  0.50

22, 23, 28

15, 16, 22, 23

6.20  2.20

1.50

2.9  2.5

0

22, 23

0

27, 28, 30

Eight Burst Planetary/ S. Ring Nebula

8, 9 15, 16

1.10  0.70

Spindle Galaxy, h 3223

4, 8, 9

Map no.

3.10  2.10

7.20  2.40

1.8 h 666

h 665

3.30  2.20 0

Name/Notes

Size

139

3258 3261 3254 3263 3269 3268 3271 3273 3275 3278 3274 3259 3277 3266

h 3256

h 3258

H I-72

h 3261

h 3264

h 3263

h 3265

h 3259

h 3266

h 3268

H II-358

H II-870

H II-359 *

H II-871

3294 3308 3300 3309

H I-164 *

h 3279

H III-55

h 3280

3293

3256

h 3254

h 3276

3245

H I-86 *

3285

3231

h 704

3366

3255

h 3253

h 3270

3250

h 3252

h 3294

3218

H I-283

3239

H IV-10 3244

3242

H IV-27 *

3247

3241

h 3249

h 4019

3227

H II-29 *

h 3250

3226

H II-28 *

HYD

LEO

HYD

LMI

CAR

VEL

HYD

UMA

LMI

UMA

LEO

ANT

ANT

ANT

ANT

ANT

ANT

VEL

LMI

VEL

ANT

VEL

LMI

UMA

CAR

ANT

DRA

CAR

ANT

LEO

HYD

ANT

LEO

LEO

10 36.6

10 36.6

10 36.4

10 36.3

10 35.8

10 35.2

10 33.6

10 33.3

10 32.9

10 32.6

10 32.3

10 31.6

10 30.9

10 30.5

10 30.5

10 30.0

10 30.0

10 29.3

10 29.3

10 29.0

10 28.9

10 27.8

10 27.3

10 26.7

10 26.5

10 26.5

10 26.5

10 25.9

10 25.5

10 25.1

10 24.8

10 24.3

10 23.5

10 23.4

27 31

þ14 10

27 26

þ37 20

58 14

43 41

27 27

þ64 45

þ28 31

þ65 03

þ27 40

39 57

36 44

35 37

35 22

35 20

35 13

44 08

þ29 30

44 39

35 36

43 54

þ28 30

þ66 48

60 40

39 57

þ74 39

57 56

39 50

þ17 10

18 38

32 29

þ19 52

þ19 54

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

OC

GX

GX/NE

OCþDN

GX

GX

PN

GX

GX

GX

11.6

12.3

12.0

11.2

4.7

11.4

12.1

12.5

11.7

12.2

12.5

12.3

11.4

12.5

11.8

11.5

12.3

11.1

11.6

11.2

11.5

11.3

10.7

–

11.0

11.2

11.8

7.6

12.3

11.1

7.7

12.1

10.4

11.4 0

0

0

0

0

0

23

h 720 h 715

1.70  0.90

0

1.90  1.60

1.7  0.9

0

1.70  1.30

3.40  1.80

h 727 ¼ h 3273

h 724

23

9, 15, 16

23

9

22, 23, 28 27, 28

5.00

23

3, 4

9

3, 4

9

22, 23, 28

1.80  0.80

2.7  1.5

0

Gem Cluster

h 717 0

h 721 1.40  1.20

2.1  1.8

0

0

2.0  1.1

0

0

1.30  0.90

2.8  2.1

22, 23

23 0

0

23 1.60  0.70

3.0  1.8

0

0

2.4  1.1

23

22, 23, 28

9

22, 23, 28

22, 23

22, 23, 28

9

3, 4

27, 28

22, 23, 28

1, 4

27, 28

22, 23, 28

9, 15, 16

15, 16, 23

3.00  2.50

h 714

h 711

h 710

Ghost of Jupiter, h 3248

22, 23

9, 15, 16

9, 15, 16

0

0

3.00  0.70

4.5  1.4

0

3.50  2.80

2.9  2.5

0

3.80  2.10

3.2  1.8

0

4.00

2.0

0

2.70  2.00

2.3  1.4

0

5.00

2.1  1.8

0

4.50  2.40

1.1

0

2.40  1.60

4.1  3.9

0

2.80  2.00

140 3370 3348 3377 3379/M 105 3450 3390 3385 3384 3393

H II-99 *

H I-17 *

h 3303

h 3298

h 760

H I-18 *

h 3299

3368/M 96

h 749

H II-81

3367

H II-78

H I-80

3359

H V-52

DRA

3329 3353

H I-284

H III-842

LEO

3351/M 95

HYD

LEO

SEX

HYD

HYD

LEO

LEO

UMA

LEO

LEO

LEO

UMA

UMA

CAR

LEO

ANT

LEO

LMI

ANT

h 743

3347

h 3291

LEO

3372

3342 ¼ 3332

H III-5 ¼ H I-272

LEO

h 3295

3338

H II-77

HYD

3346

3336

h 3289

UMA

H V-7

3320

H II-745

UMA

3358

3319

H III-700

UMA

VEL

h 3293

3310

H IV-60 *

3344

3330

h 3287

CAR

VEL

3345

3324

h 3286

H I-81 *

3318

h 3285

HYD

LEO

HYD

Con

H I-26

3301 3312

H II-46

3311

h 3281

h 3282

NGC/M

Herschel

10 48.3

10 48.3

10 48.2

10 48.1

10 48.1

10 47.8

10 47.7

10 47.2

10 47.1

10 46.8

10 46.6

10 46.6

10 45.4

10 44.7

10 44.0

10 43.8

10 43.7

10 43.6

10 43.6

10 43.5

10 42.8

10 42.7

10 42.1

10 40.3

10 39.6

10 39.2

10 38.7

10 38.6

10 37.3

10 37.3

10 37.0

10 36.9

10 36.7

25 10

þ12 38

þ04 55

31 32

20 51

þ12 35

þ13 59

þ72 50

þ17 16

þ11 49

þ13 45

þ63 13

þ55 58

þ76 49

þ11 42

59 52

þ14 52

36 23

þ11 59

þ24 55

36 22

þ09 26

þ13 45

27 46

þ47 24

þ41 41

þ53 30

54 09

58 38

41 38

27 34

þ21 53

27 32

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

DN

GX

GX

NE

GX

GX

GX

GX

GX

GX

GX

GX

OC

OCþDN

GX

GX

GX

GX

Type

12.2

9.9

12.4

12.1

11.9

9.5

10.2

11.1

11.7

9.3

11.4

10.3

12.4

12.2

9.8

3.0p

11.8

11.5

–

9.7

11.4

12.5

10.9

12.3

12.4

10.8

10.6

7.4

6.7

11.5

11.9

11.4

11.6

Mag

0

0

h 739

9

h 741 h 745

7.20  4.40 0

0

h 757

5.30  4.80

23 0

1.80  1.50

5.40  2.70

1.5  0.9

0

23

9, 15, 16

15, 16

23

2.6  2.3

3.50  0.60

9, 15, 16

9, 15, 16

1, 4

9, 15, 16

9, 15, 16

9, 15, 16

3, 4

4

1, 4

9, 15, 16

0

0

h 758

h 754

0

0

5.0  3.0

h 738

h 750 2.00

2.6  1.5

0

7.80  5.20

2.5  2.4

0

h 748

h 733 1.40  1.00

1.9  1.1

0

0

27, 28

Eta Carinae Nebula

120.00 7.40  5.00

23 9, 15, 16

h 3290

2.70  2.60

9, 15, 16

3.20  1.80

–

7.1  6.5

likely a double star

23

0

3.40  2.10 0

9, 15, 16

1.40

23 9, 15, 16

5.70  3.40 h 737

2.00  1.60

4, 8, 9 4, 9

h 732

4

28

27, 28

22, 23, 28

23

9

23

Map no.

2.20  1.00

h 731

h 728

Name/Notes

6.10  3.40

3.10  2.40

6.0

0

16.00  14.00

2.3  1.2

0

3.30  1.20

3.3  1.0

0

22.30  2.10

Size

141

3430 3432 3437 3449 3403 3456 3455 3445 3448 3457 3462 3458

H I-118

H I-172 *

H II-47

h 3302

H II-335

H IV-29

H II-82

H I-267

H I-233

h 793

H II-16

H I-268

3485 3489 3486 3495

H II-100

H II-101 *

H I-87 *

H III-498

3496

3446

h 3301

h 3310

3433

H III-20

3483

3434

H III-497

3471

3424

H II-494

H III-972

3415

h 3307

3414

3412

H I- 27 *

H II-718

3394

H II-872

H II-362 *

3411

H III-522

3423

3396

H I-117

3413

3395

H I-116 *

H II-493

3389

H II-41

H II-131 ¼ H IV 6

3381

H II-565

LEO

LMI

LEO

LEO

CAR

UMA

HYD

UMA

LEO

LEO

UMA

UMA

LEO

CRT

DRA

ANT

LEO

LMI

LMI

VEL

LEO

LEO

LMI

UMA

LMI

LMI

SEX

LEO

UMA

HYD

LMI

LMI

LEO

LMI

11 01.3

11 00.4

11 00.3

11 00.0

10 59.8

10 59.1

10 59.0

10 56.0

10 55.3

10 54.7

10 54.7

10 54.6

10 54.5

10 54.1

10 53.9

10 52.9

10 52.6

10 52.5

10 52.2

10 52.1

10 52.1

10 52.0

10 51.8

10 51.7

10 51.3

10 51.3

10 51.2

10 50.9

10 50.6

10 50.3

10 49.9

10 49.8

10 48.5

10 48.4

þ03 38

þ28 58

þ13 54

þ14 50

60 20

þ61 32

28 28

þ57 07

þ07 42

þ17 37

þ54 19

þ56 59

þ17 17

16 02

þ73 41

32 56

þ22 56

þ36 37

þ32 57

45 09

þ10 09

þ03 48

þ32 54

þ43 43

þ27 59

þ32 46

þ05 50

þ13 25

þ65 43

12 51

þ32 59

þ32 59

þ12 32

þ34 42

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

12.0

10.3

10.2

11.9

8.2

12.3

12.2

12.3

12.3

12.3

11.6

12.3

12.3

12.6

12.2

11.7

12.1

11.1

11.5

–

11.8

12.3

12.4

12.4

10.9

12.1

10.9

10.4

12.4

11.9

12.0

11.8

11.8

11.8

h 773 h 772

2.10  1.30

h 767 h 792

1.70  1.20

0

h 3309 h 805 h 809

7.1  5.2

4.90  1.10

h 806 0

0

3.60  2.20

2.4  2.2

0

16

9

9, 15, 16

9, 15, 16

27, 28 0

3, 4

23

4

15, 16

7.00

0

h 794

9, 15, 16

4

4

9, 15, 16

16, 23

1, 4

23

9

9

9

23, 18

9, 15, 16

15, 16

9

4, 9

9

9

9, 15, 16

9, 15, 16

3, 4

15, 16, 13

9

9

9, 15, 16

9

1.70  0.80

1.8  1.2

0

1.40  0.80

1.7  1.2

0

0.90

5.6  1.7

0

h 788

h 787 0

h 791 1.60  1.40

2.6  2.0

0

0

3.0  1.3

0

0

3.30  1.00

2.6  0.8

0

h 786

h 780 0

h 779

6.60  1.60

4.1  2.2

0

0

6.50

3.5  3.0

0

h 783

h 784

0

h 778

2.10  1.90

2.7  0.8

0

0

3.5  2.6

0

0

1.80  0.80

3.9  3.3

0

h 777

h 774

3.70  2.20 0

h 764

0

0

1.9  1.4

h 776

2.10

2.9  1.2

0

h 766

h 765

0

h 761

2.9  1.3 2.10  1.10

h 756

0

0

2.00  1.80

142 3583 3593 3587/M 97 3596 3603

H II-728

H I-29 *

h 838

H II-102

h 3334

CAR

3590

H II-337 3585

3584 3562

h 3329

h 3332

3582

h 3327

H II-269

DRA

3581

h 3326

CAR

LEO

UMA

LEO

UMA

HYD

CAR

CAR

CAR

CAR

CAR

CRA

UMA

UMA

CEN

CEN

CAR

3579

3564

h 3320

3576

3572

h 3323

CEN

h 3325

3557

h 3319

LEO

h 3324

3547

H II-42

CRA

3571

3528

h 3316

UMA

3556/M 108

3516

H II-336

CAR

H II-819

3532

h 3315

LEO

H V-46 *

3521

H I-13 *

CAR

3568

3519

h 3314

LMI

3549

3512

H II-366

CRT

H I-220

3513

H V-40

LEO

CRT

LMI

UMA

CAR

Con

h 3321

3511

3504

H I-88 * 3507

3488

H I-269

H V-39

3503

h 3311

H IV-7

NGC/M

Herschel

11 15.1

11 15.1

11 14.8

11 14.6

11 14.2

11 13.3

11 12.9

11 12.9

11 12.4

11 12.3

11 12.1

11 11.9

11 11.8

11 11.5

11 11.5

11 10.9

11 10.8

11 10.6

11 10.4

11 10.0

11 09.9

11 07.3

11 06.8

11 06.4

11 05.8

11 04.0

11 04.0

11 03.8

11 03.5

11 03.4

11 03.2

11 01.4

11 01.3

61 15

þ14 47

þ55 01

þ12 49

þ48 19

26 45

60 47

þ72 53

61 12

61 16

61 18

61 14

61 23

18 17

þ55 40

þ53 23

37 27

37 33

60 14

37 32

þ10 43

19 28

þ72 34

58 40

00 02

61 22

þ28 02

23 15

þ18 08

23 05

þ27 58

þ57 41

59 51

RA (2000.0) Dec

OCþDN

GX

PN

GX

GX

GX

OC

GX

DN

DN

DN

DN

DN

GX

GX

GX

GX

GX

OCþDN

GX

GX

GX

GX

OC

GX

OC/NE

GX

GX

GX

GX

GX

GX

DN

Type

9.1

10.9

9.9

11.0

11.2

9.9

8.2

12.2

–

–

–

–

–

12.2

9.9

12.1

12.3

12.2

6.6

10.6

12.3

11.6

11.5

3.0

9.2

7.7

12.3

11.1

11.9

10.8

10.9

12.9

–

Mag

0

0

2.0

28

h 841

4.00  3.80 4.0

0

Owl Nebula

2.80

28

9, 16

4

4, 9 9, 16

h 840

5.20  1.90

23 2.80  1.80

4.60  2.50

h 3328

1, 4 0

28

28

28

28

28

16, 23

4

– h 830

h 831

4

23

23

27, 28

23

1.70  1.30

–

–

20.00  15.00

3.0

0

3.00  0.90

8.6  2.4

0

3.10  1.00

2.5  0.9

0

1.70  0.90

7.0

0

4.00  3.00

16, 13 9, 16

2.00  0.90

h 828

2.60  1.50

28 1, 4

1.90  1.40 h 816

50.00

27, 28 16

11.20  5.40 h 818

8.00

23 9

h 815

23 9, 16

1.60  1.50

h 812

2.90  2.40

3.40  2.90

6.0  2.1

0

0

h 810

9

4

h 803

2.70  2.10

1.8  1.2

0

3.0

27, 28

Map no.

0

Name/Notes

0

Size

143

3660 3659 3662 3657 3658 3666

H II-635

H II-53

H IV-4

H III-768

H IV-59

H I-20

3656

3642

H I-245

H II-782

3646

H III-15

3655

3645

H II-32

H I-5 *

UMA

3640

H II-33 *

3648

3631

H I-226 *

3652

3629

H II-338

h 868

3636

H II-550

H II-775

UMA

3630

LEO

UMA

UMA

LEO

LEO

CRA

UMA

LEO

UMA

LEO

LEO

LEO

UMA

LEO

CRT

LEO

LEO

LEO

LEO

UMA

LEO

UMA

UMA

h 861

3613

H I-271 *

3628

3610

H I-270 *

HYD

UMA

H V-8 *

3621

H I-241 *

3627/M 66

3614

H II-729

LEO

LEO

3626

3611

H II-521

h 857 ¼ h 875

3608

H II-51 *

LEO

LEO

H II-52 *

3607

H II-50 *

3623/M 65

3605

H III-27

UMA

LEO

3619

3600

H II-709

H I-244 *

3599

H II-49

UMA

h 854

3595

H III-706

11 24.4

11 24.0

11 23.9

11 23.8

11 23.8

11 23.6

11 23.6

11 22.9

11 22.6

11 22.6

11 22.3

11 21.7

11 21.6

11 21.1

11 21.0

11 20.5

11 20.4

11 20.3

11 20.3

11 20.2

11 20.1

11 19.4

11 18.9

11 18.6

11 18.4

11 18.3

11 18.3

11 17.5

11 17.0

11 16.9

11 16.8

11 15.8

11 15.4

11 15.4

þ11 21

þ38 34

þ52 55

01 06

þ17 49

08 40

þ53 51

þ16 35

þ37 46

þ39 53

þ59 05

þ20 10

þ02 59

þ03 14

þ53 10

þ26 58

10 17

þ02 58

þ13 36

þ12 59

þ18 21

þ57 46

þ13 05

þ58 00

þ58 47

32 49

þ45 45

þ04 33

þ18 09

þ18 03

þ18 01

þ41 36

þ18 07

þ47 27

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

11.7

12.1

12.3

13.0

12.2

12.2

12.3

11.6

12.1

12.5

10.8

10.8

12.1

10.3

10.1

12.2

12.4

12.1

9.6

8.9

10.9

11.5

9.2

10.8

10.7

9.4

11.6

11.9

10.7

9.9

12.1

11.7

11.8

12.1 h 843 h 842

4.10  0.80 h 844 h 845

4.60  4.00

0

h 864 h 867

2.00  0.80

h 866 h 865

5.50  4.70

h 874

1.60

h 877 h 882

1.8  1.7

4.40  1.00

h 876

1.10  0.70 0

h 879

1.30  0.80 0

h 878

2.30  1.30

2.8  2.3

0

0

h 873

1.50  1.00

9, 16

9

4

16

9, 16

16

4

9, 16

9 9

h 871

1.3  0.8

2.60  0.70

4

9

16

16

4

0

0

3.9  2.2

0

0

4.0  3.2

0

h 858

5.00  3.70 0

h 860

2.30  1.60

9

16 16

h 862

9, 16

1.30

member Leo Triplet, h 859

13.10  3.10

9, 16

9, 16

4

9, 16

4

4

23

4, 9

16

9, 16

9, 16

9, 16

4, 9

9, 16

4, 9

2.00  0.80

member Leo Triplet

h 856

h 852

9.10  4.10

2.7  1.9

0

2.70  2.30

9.8  2.9

0

member Leo Triplet

h 848

0

h 847

2.7  2.3 3.90  1.90

h 3337

0

0

12.30  6.80

4.6  2.6

0

h 850

h 849

0

h 846

2.00  1.60

3.2  2.6

0

0

1.4  0.9

0

0

2.7  2.1

0

0

1.60  0.70

144 UMA CEN

3668 3680 3675 3674 3681 3684 3683 3682 3686 3687

H II-845

h 3342

H I-194 *

H II-886

H II-159

h 893

H I-246

H I-262

H II-160 ¼ H III-28 *

H II-770

HYD

3733 3742 3738 3735 3766 3756

H II-783

H I-287

h 3352

H II-784

3732

H II-552

H III-771

3729

H I-222 *

h 3350

3726

3715

H II-562

H II-730 *

HYD

3705

H II-13 3717

3706

h 3346

3718

3690

H I-247

h 3348

3692

H II-152

H I-221

CRT

3691

H II-54

UMA

CEN

DRA

UMA

CEN

UMA

CRT

UMA

UMA

UMA

LEO

CEN

UMA

LEO

LEO

LEO

3699 3689

h 3345

H II-339

LEO

DRA

UMA

LEO

LEO

UMA

UMA

CEN

UMA

UMA

3673

CRT

3669

3672

H I-131

UMA

h 3341

3665

H I-219 *

Con

H II-829

NGC/M

Herschel

11 36.8

11 36.1

11 36.0

11 35.8

11 35.4

11 35.0

11 34.2

11 33.8

11 33.3

11 32.6

11 31.5

11 31.5

11 30.1

11 29.7

11 28.5

11 28.4

11 28.2

11 28.2

11 28.0

11 28.0

11 27.7

11 27.7

11 27.5

11 27.2

11 26.5

11 26.4

11 26.1

11 25.7

11 25.5

11 25.4

11 25.2

11 25.0

11 24.7

þ54 18

61 37

þ70 32

þ54 31

37 56

þ54 51

09 51

þ53 08

þ47 02

þ53 04

30 19

14 12

þ09 17

36 25

þ58 33

þ09 24

þ16 55

þ25 40

59 57

þ29 31

þ17 13

þ66 35

þ56 53

þ17 02

þ16 52

þ57 03

þ43 35

43 15

þ63 27

þ57 43

26 44

09 48

þ38 46

RA (2000.0) Dec

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

PN

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

Type

11.2

5.3

11.9

11.5

12.2

11.8

12.5

11.0

10.2

10.6

11.4

12.5

11.0

11.4

11.2

12.1

12.4

12.3

11.3

12.1

11.2

12.4

12.5

11.5

11.6

12.2

10.0

7.6

12.3

12.4

11.5

11.4

10.7

Mag

h 886

4.00  1.80

0

0

0

h 913

h 914 Pearl Cluster h 918

15.00 4.20  2.10

0

4.00  0.80

2.5  1.9

0

2.40  1.70

4.9  2.2

0

0

h 911

2.9  1.9

1.40  1.20

h 910 0

6.00  4.10 0

h 908

0

h 3347

h 902 ¼ h 903

8.10  4.00

6.2  1.0

0

1.40  0.90

4.9  2.0

0

3.10  1.80

1.6  1.4

0

h 896

h 898

1.40  1.00 3.10  0.70

h 897

h 895

1.70  1.10

0.8

0

1.90

3.1  2.4

0

h 894

h 890

0

h 892

1.8  0.7 1.70  1.10

h 891 ¼ h 3343

h 887

0

0

3.10  2.10

3.0  2.2

0

1.70  0.60

5.9  3.1

0

0

h 880

1.70  1.30 7.00

h 883

3.7  2.4 2.00  0.50

0

h 881

4.30  3.30 0

Name/Notes

Size

4

28

1, 4

4

23

4

16

4

4,9

4

23

16, 23

16

23

4

16

9, 16

9

28

9

9, 16

4

4

9, 16

9, 16

4

4, 9

23, 28

4

4

23

16

9

Map no.

145

UMA UMA

3769 3773 3783 3782 3780

H II-731

H III-81

h 3354

H II-732

H I-227

3900 3904

H I-82 *

H II-864

3917

3898

H I-228 *

H II-824

3894

H I-248

3918

3893

H II-738 *

h 3365

3892

H II-553

3909

3888

H II-785

3912

3887

H I-120

h 3364

3885

H III-828

H II-342 *

3877 3882

H I-201 *

3870

H III-833

h 3358

3872

3842

H III-377

H II-104

UMA

3818

H III-284 3835

3813

H I-94 *

3838

3811

H II-737

h 958

3810

H I-21 *

H II-831

LEO

3801

H II-161

UMA

CEN

LEO

CEN

HYD

LEO

UMA

UMA

UMA

CRT

UMA

CRA

HYD

CEN

UMA

UMA

LEO

UMA

VIR

UMA

UMA

LEO

LEO

LEO

3786 3800

h 931

H II-103

UMA

CEN

LEO

UMA

LEO

3768

H III-29

UMA

3757

H III-843

11 50.8

11 50.3

11 50.1

11 49.6

11 49.2

11 49.2

11 49.2

11 48.8

11 48.6

11 48.0

11 47.6

11 47.1

11 46.8

11 46.1

11 46.1

11 45.9

11 45.8

11 44.2

11 44.1

11 44.0

11 42.0

11 41.3

11 41.3

11 41.0

11 40.3

11 40.2

11 39.7

11 39.4

11 39.3

11 39.0

11 38.2

11 37.7

11 37.2

11 37.1

þ51 50

57 11

þ26 29

48 15

29 17

þ27 01

þ56 05

þ59 25

þ48 43

10 58

þ55 58

16 51

27 55

56 22

þ47 30

þ50 12

þ13 46

þ57 57

þ60 07

þ19 57

06 09

þ36 33

þ47 42

þ11 28

þ17 44

þ15 21

þ31 55

þ56 16

þ46 31

37 45

þ12 07

þ47 54

þ17 51

þ58 26

GX

PN

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

11.8

8.1

12.6

–

10.8

11.4

10.8

11.6

10.2

11.5

12.0

10.6

11.1

12.5

11.2

12.4

11.7

12.3

12.3

11.8

11.7

11.5

12.2

10.6

12.0

12.5

12.4

11.5

12.4

11.6

12.3

11.5

12.5

12.5

h 929

h 942 h 945 h 948 h 962

1.40  1.00

h 3363

2.70  2.00

h 992 Blue Planetary h 994

0.40 5.00  1.10

20.0

1.50  0.90

0

4.4  2.6

h 988

h 983

2.80  1.70

h 985

h 982

4.50  2.80

3.20  1.70

h 981 ¼ h 3361

3.10  2.30

0

h 978

1.80  1.40

0

h 979 ¼ h 3360

0

3.50  2.70

2.4  1.0

0

2.30  1.40

5.3  1.2

0

h 3359

h 972

1.00  0.80 0

h 973

1.90  1.20

4

28

9

23, 28

23

9

4

4

4, 9

16, 23

4

16, 23

23

28

4, 9

4, 9

9, 16

4 4

h 959

1.8  0.7 1.40  0.60

9, 16

16

9

4, 9

9, 16

9, 16

9, 16

9

4

4, 9

23

9, 16

4, 9

9, 16

4

0

0

2.0  1.2

0

0

2.2  1.7 2.00  1.00

h 943

4.30  3.00 0

h 939

2.50  1.60 0

h 936 ¼ h 3356

2.00  0.60

2.1  1.1

0

0

h 930

3.00  2.40

1.6  1.1

0

0

1.90  1.70

1.2  1.0

0

h 928

h 925

2.90  1.00 0

h 923

0

1.6  0.9

h 919 0

1.10

146 3972 3976 3981 3978 3982 3990 3992/M 109 3998 4008 4013 4024 4010 4014 4020 4026 4027

H II-789

H III-274

H II-840

H IV-62 *

H II-791

H IV-61 *

H I-229 *

H II-368

h 1041

H II-295

h 1040

h 1042

h 1045

H I-223 *

H II-296 *

3968

H II-162

H II-132

3963

3953

H V-45 *

H IV-67

3949

H I-202 *

3962

3945

H I-251 *

H I-67 *

3941

H I-173 *

3955

3938

H I-203 *

H II-623

CRT

3937

H III-389

3957

3936

h 3367

3956

3928

H II-740

H II-294

3921

H II-788

H III-290

UMA

3923

H I-259

CRV

UMA

UMA

COM

UMA

CRV

UMA

LEO

UMA

UMA

UMA

UMA

UMA

CRT

VIR

UMA

LEO

UMA

CRT

CRT

CRT

UMA

UMA

UMA

UMA

LEO

HYD

UMA

UMA

HYD

CEN

3960

h 3369

Con

NGC/M

Herschel

11 59.5

11 59.4

11 58.9

11 58.6

11 58.6

11 58.5

11 58.5

11 58.3

11 57.9

11 57.6

11 57.6

11 56.5

11 56.2

11 56.1

11 56.0

11 55.8

11 55.5

11 55.0

11 54.7

11 54.0

11 54.0

11 54.0

11 53.8

11 53.7

11 53.2

11 52.9

11 52.8

11 52.7

11 52.3

11 51.8

11 51.1

11 51.0

11 50.9

19 16

þ50 58

þ30 25

þ16 11

þ47 16

18 21

þ43 57

þ28 12

þ55 27

þ53 23

þ55 28

þ55 08

þ60 31

19 54

þ06 45

þ55 19

þ11 58

þ58 30

13 58

23 10

20 34

19 34

þ52 20

þ47 52

þ60 41

þ36 59

þ44 07

þ20 39

26 54

þ48 41

þ55 05

28 48

55 42

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

Type

11.0

10.7

12.5

12.4

12.3

11.7

11.5

11.9

10.6

9.8

12.5

11.1

12.4

11.0

11.7

12.1

11.9

11.7

10.7

11.7

12.2

12.1

9.8

10.6

10.5

10.3

10.1

12.5

11.9

12.2

12.2

9.6

8.3

Mag

h 1003 h 1002 h 1005 h 1006

5.20  3.50

3.7  1.0

4

0

0

h 1047 h 3371

3.30  2.40

5.2  1.3

0

0

1.90  1.00

1.4  0.9

0

4.20  0.90

1.9  1.6

0

5.20  1.00

2.4  1.3

0

h 1038

h 1031 0

h 1030 2.70  2.30

7.5  4.4

0

h 1029

1.40  0.80 0

h 1017

2.30  2.00

16, 23

4, 9

9

9, 16

4, 9

16, 23

4, 9

9

4

4

4

4

16, 23 4

h 1023

16 1.70  1.50

h 1022

9, 16

5.30  2.50

3.80  1.20

0

h 1018

2.70  1.90 0

h 1015

2.70  2.40

4

23 16, 23

h 3370

2.60  2.20

23

16, 23

4

4, 9

4

9

4, 9

9

23

4, 9

4

3.10  1.00

3.30  1.00

2.9  0.7

0

h 3368

h 1011

0

h 1009

6.90  3.60

2.9  1.7

0

0

3.5  2.5

0

0

1.8  1.6 5.40  4.90

h 999 0

0

3.90  0.70

1.5

0

h 997

h 3366

23

2.10  1.30

5.9  3.9

28 0

Map no.

0

Name/Notes

7.00

Size

147

4104 4105

H II-370

H II-865

4124 4123 4127 4128 4133

H II-60 ¼ H I-33

H V-4

H I-279

H I-263

H I-278

4112

4102

H I-225 *

h 3380

4100

H III-717

4111

4096

H I-207

4106

4094

h 3376

H I-195 *

4087

H III-754

H II-866

4088

H I-206 *

4103

4085

H I-224 *

4108

4073

H II-277

h 3377

4062

H I-174

h 1087

4068

H II-781

CRV

4047

H II-741 4050

4045

H II-276

4051

4041

H I-252 *

H II-509

4052

h 3373

H IV-56 *

UMA

4039

H IV-28.2

UMA

DRA

DRA

CAM

VIR

VIR

CEN

CVN

HYD

DRA

CRU

HYD

COM

UMA

UMA

UMA

CRV

HYD

UMA

UMA

VIR

UMA

UMA

UMA

VIR

UMA

CRU

CRV

CRV

4036

CRV

COM

4038

4033

H II-508

H IV-28.1*

4032

H II-404

VIR

H I-253 *

4030

H I-121 *

12 08.6

12 08.5

12 08.4

12 08.2

12 08.2

12 07.1

12 07.1

12 06.8

12 06.8

12 06.7

12 06.7

12 06.6

12 06.4

12 06.2

12 06.0

12 05.9

12 05.6

12 05.6

12 05.4

12 04.5

12 04.1

12 04.0

12 03.2

12 02.9

12 02.9

12 02.7

12 02.2

12 01.9

12 01.9

12 01.9

12 01.4

12 00.6

12 00.6

12 00.4

þ74 56

þ68 46

þ76 48

þ02 53

þ10 23

40 11

þ43 04

29 46

þ67 10

61 15

29 46

þ28 10

þ52 43

þ49 35

þ47 29

14 32

26 33

þ50 33

þ50 21

þ01 54

þ31 54

þ52 35

þ44 32

16 22

þ48 38

þ01 59

þ62 08

63 12

18 53

18 52

þ61 54

17 51

þ20 04

01 06

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

12.3

11.9

12.7

11.0

11.3

12.0

10.8

11.4

12.3

7.4

10.5

12.1

11.3

11.1

10.8

12.0

12.1

10.3

12.0

11.4

11.2

12.5

10.0

12.2

12.3

11.9

11.1

8.8

10.4

10.3

10.5

11.6

12.2

10.6 0

3.0  2.0

16, 23

0

4, 9

h 1086 h 3378

2.80  2.10

h 3379 h 1088

4.60  1.00

1.8  1.3

0

0

2.40  0.90

2.5  1.2

0

h 1100

h 1096

h 1092 0

h 1094 4.30  3.20

4.3  1.4

0

0

1.60  0.90

1.6  1.3

0

0

1.70  1.40

6.0

0

2.6  1.6

0

h 1085

3.10  1.70 0

h 1084

5.40  1.70

1, 4

4

1, 4

16

16, 31

23

4, 9

23

4

28

23

9

4

4, 9

16, 23 4, 9

h 1081

23 6.50  1.80

h 3375

4, 9

4.10  1.50

2.10  1.70

5.6  2.1

0

16

h 1072

3.20  2.30 2.80  0.80

4 9

h 1066

4, 9

4.00  1.80

h 1061

4, 9

2.50  1.60

5.20  3.90

0

h 1058

1.60  1.30 0

h 1057

2.70  1.70

16

28 4

h 1054

2.70  2.60

16, 23

16, 23

4

16, 23

9, 16

16

10.00

Antennae/Ringtail Galaxy, h 1053

3.30  1.70

h 1050 Antennae/Ringtail Galaxy, h 1052

0

h 1049

h 1048

3.40  1.70

4.3  1.7

0

2.40  1.20

1.6  1.2

0

4.20  3.20

148 4203 4210 4206 4214 4213 4212 ¼ 4208 4218 4217

H III-850

H II-165

H I-95 *

H II-354

H II-108 ¼ H II-107

H III-718

H II-748

4185

H II-373

4194

4183

H III-697

H I-175 *

4179

H I-9 *

H II-867

4177

H III-534

4193

4178

h 1125

4189

4168

H II-105

H II-163

4169

H III-358

H II-106

4162

H II-353

4184

4158

H II-405

4192/M 98

4157

H I-208

h 3384

4152

h 1132

4150

4145

H I-169

H II-83

4144

H II-747

H I-73 *

4143

H IV-54 *

4147 ¼ 4153

4138

H I-196

4151

4136

H II-321

H I-165 *

4129

H II-548

H I-19 * ¼ H I-11

NGC/M

Herschel

CVN

CVN

COM

COM

CVN

VIR

DRA

COM

UMA

VIR

COM

COM

CRU

COM

CVN

VIR

CRV

VIR

VIR

COM

COM

COM

UMA

COM

COM

CVN

COM

CVN

UMA

CVN

CVN

COM

VIR

Con

12 15.8

12 15.8

12 15.7

12 15.7

12 15.6

12 15.3

12 15.3

12 15.1

12 14.2

12 13.9

12 13.8

12 13.8

12 13.6

12 13.4

12 13.3

12 12.9

12 12.8

12 12.8

12 12.3

12 12.2

12 11.9

12 11.2

12 11.1

12 10.6

12 10.6

12 10.5

12 10.1

12 10.0

12 10.0

12 09.6

12 09.5

12 09.3

12 08.9

þ47 06

þ48 08

þ13 54

þ23 59

þ36 20

þ13 02

þ65 59

þ33 12

þ54 32

þ13 10

þ13 26

þ14 54

62 42

þ28 31

þ43 42

þ01 18

14 00

þ10 52

þ13 12

þ29 10

þ24 07

þ20 11

þ50 29

þ16 02

þ30 24

þ39 24

þ18 33

þ39 53

þ46 27

þ42 32

þ43 41

þ29 56

09 02

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

Type

11.3

12.5

11.1

12.5

9.6

12.0

12.5

10.7

12.4

12.4

11.8

10.1

–

12.4

12.1

10.9

12.5

11.3

11.2

12.2

12.0

12.1

11.3

11.9

11.4

10.3

10.4

10.8

11.3

10.8

11.3

11.1

12.5

Mag 16

h 1110 h 1112 h 1114 h 1115

2.00  1.80

h 3383 h 1126

4.20  1.30

h 1128 h 1129

2.60  2.00

h 1131 h 1134

2.20  1.10

5.2  1.5

0

0

h 1149

h 1144 1.20  0.70

3.2  2.0

0

0

h 1146 h 1145

0

1.70

8.0  6.6

0

6.40  1.10

2.0  1.6

0

h 1143

h 1140 0

h 1135 3.50  3.20

2.7  1.6

0

0

2.5  1.7

0

0

9.80  2.80

2.0

0

5.3  0.7

0

0

1.7  1.2

0

0

5.00  1.70

2.8  2.2

0

h 1119

h 1120 0

h 1117

1.80  0.90

2.3  1.4

0

0

6.7  1.2

0

0

2.3  1.6 2.30  1.90

h 1111

0

0

6.30  4.50

4.4 h 1106

h 1105

5.90  4.10 0

h 1107

6.10  1.50

4, 9

4, 9

9, 16, 31

9

9

9, 16, 31

4

9

4

9, 16, 31

9, 16, 31

9, 16, 31

28

9

4, 9

16

16, 23

9, 16, 31

9, 16, 31

9

9

9

4, 9

9, 16, 31

9

9

9, 16

9

4, 9

4, 9 4, 9

9

h 1104

h 1108

3.90  3.60 2.30  1.40

h 1097 ¼ h 3382

2.30  0.60

Map no.

2.60  1.70

Name/Notes

Size

149

4262 4271 4274 4267 4270 4273 4278

H II-110

H II-804

H I-75 *

H II-166

H II-568

H II-569 *

H I-90 ¼ H II-322 *

4290

4261

H II-139 *

4281

4260

H II-138

H II-805

4258/M 106

H V-43 *

H II-573 ¼ H II-570 *

4254/M 99

h 1173

4283

4256

H II-846

H II-323 ¼ H II-377

4251

H I-89 *

4291

4248

H II-742

H I-275

4245

H I-74 *

4235

H II-17

4244

4237

H II-11

H V-41

4233

H II-496

4242

4236

H V-51

H III-725

CEN

4224

H II-136

4230

4223

H II-137

4250

4219

h 3385

h 3386

4220

H I-209

H I-264

VIR

4221

h 1150

UMA

VIR

COM

DRA

COM

VIR

VIR

VIR

COM

UMA

COM

VIR

VIR

CVN

COM

DRA

COM

CVN

COM

CVN

CVN

DRA

COM

VIR

DRA

VIR

VIR

CEN

CVN

DRA

VIR

4215

H II-135

VIR

4216

H I-35 *

12 20.8

12 20.4

12 20.3

12 20.3

12 20.1

12 19.9

12 19.8

12 19.8

12 19.8

12 19.6

12 19.5

12 19.4

12 19.4

12 19.0

12 18.8

12 18.7

12 18.1

12 17.8

12 17.6

12 17.5

12 17.5

12 17.4

12 17.3

12 17.2

12 17.2

12 17.1

12 16.7

12 16.6

12 16.5

12 16.4

12 16.2

12 16.0

12 15.9

12 15.9

þ58 06

þ05 23

þ29 19

þ75 22

þ29 17

þ05 21

þ05 28

þ12 48

þ29 37

þ56 45

þ14 53

þ05 49

þ06 06

þ47 18

þ14 25

þ65 54

þ28 10

þ47 25

þ29 36

þ37 49

þ45 37

þ70 48

55 08

þ07 11

þ15 19

þ07 37

þ69 28

þ07 28

þ06 42

43 20

þ47 53

þ66 14

þ06 24

þ13 09

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX/NE

GX

GX

GX

GX

GX

12.0

11.4

12.0

11.4

10.1

11.7

12.1

10.8

10.5

12.5

11.5

10.4

11.8

8.3

9.7

11.9

10.6

12.4

11.4

10.0

10.9

11.9

9.0p

11.7

11.8

12.0

10.1

12.0

12.1

11.9

11.3

12.5

11.4

10.3 0

0

h 1163

0

h 1159

0

2.20  1.60

3.0  1.6

0

h 1193

h 1187 ¼ h 1194

h 1188 0

h 1192 1.50

h 1186

3.80 2.00  1.70

h 1183 ¼ h 1189

2.30  1.50

2.0  0.9

0

h 2849

h 1181 0

h 1185 3.00  2.80

6.8  2.4

0

0

1.50  1.30

1.8  1.6

0

h 1179

h 1176 0

h 1177

2.7  1.3

4.10  3.60

h 1175

Pinwheel Galaxy 0

0

18.60  7.20

5.3  4.6

0

4.10

3.6  1.5

0

h 1171

h 1169 0

h 1168

2.9  2.2 2.90  1.20

h 1167

16.60  1.90 0

h 1166

5.20  4.00 0

h 1170

2.70  2.10

7.0  5.0

0

0

h 1162

4.20  0.90

2.1  1.4

0

0

2.40  1.10

21.9  7.2 h 1161

h 1153 0

h 1152

2.5  1.4 2.50  1.00

h 1151

h 1147

h 1148

0

0

3.70  1.10

3.9  1.5

0

2.20  1.70

1.8  0.7

0

8.10  1.80

4

16, 31

9

1, 4

9

16, 31

16, 31

9, 16, 31

9

4

9, 16, 31

16, 31

16, 31

4, 9

9, 16, 31

4

9

4, 9

9

9

4, 9

1, 4

28

16, 31

9, 16, 31

16, 31

4

16, 31

16, 31

28

4, 9

4

16, 31

9, 16, 31

150 DRA COM

4313 4332

4348 4337 4350 4352 4386 4365 4361

H II-625

h 3388

H II-86 *

H II-64

H I-277

H I-30 *

H I-65 *

4371

4343

H III-94

H I-22 *

CRU

4339

H II-143

4349

4342

H III-96

4369

4340

H II-85

h 3389

4344

H III-31

H I-166

CRV

4346

H I-210 *

VIR

CVN

VIR

DRA

VIR

COM

CRU

VIR

VIR

VIR

VIR

COM

COM

CVN

UMA

4321/M 100 4335

h 1211

H II-806

VIR

COM

COM

COM

HYD

VIR

VIR

H II-847

4305

h 1203

H II-63

4303/M 61

H I-139 *

VIR

COM

4314

4299

H II-62

H I-76 *

4302

H II-112

DRA

COM

4312

4319

H I-276

H II-628

4298

H II-111

VIR

VIR

4304

4292

h 1196

4310

4294

H II-61

COM

H II-378

4293

H V-5 *

Con

h 3387

NGC/M

Herschel

12 24.9

12 24.6

12 24.5

12 24.5

12 24.5

12 24.5

12 24.1

12 24.0

12 23.9

12 23.9

12 23.7

12 23.6

12 23.6

12 23.6

12 23.6

12 23.5

12 23.0

12 22.9

12 22.8

12 22.6

12 22.6

12 22.5

12 22.4

12 22.2

12 22.1

12 21.9

12 21.7

12 21.7

12 21.7

12 21.5

12 21.3

12 21.3

12 21.2

þ11 42

þ39 23

61 54

18 48

þ07 19

þ75 32

þ11 13

þ16 42

58 08

03 27

þ06 57

þ06 05

þ07 03

þ16 43

þ17 32

þ47 00

þ58 27

þ15 49

þ65 51

þ11 48

þ29 53

þ15 32

þ29 12

33 29

þ12 44

þ04 28

þ11 30

þ14 36

þ75 19

þ14 36

þ04 36

þ11 31

þ18 23

RA (2000.0) Dec

GX

GX

OC

PN

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

Type

11.0

11.4

7.4

10.9

9.6

11.7

12.5

11.0

8.9

12.5

12.4

11.3

12.2

11.2

12.4

11.3

12.4

9.3

12.2

12.0

10.5

11.8

12.4

11.6

12.4

9.3

12.3

11.9

12.0

11.4

12.2

11.8

10.3

Mag

h 1198 h 1210

2.80  2.10

h 1216

h 1221 h 1227

2.00  1.00

h 1247 h 1232 h 1231

6.90  5.00 2.10

h 1234 h 1235

2.10  2.00 4.00  2.30

4.0

0

2.5  1.3

0

0

2.9  1.6

0

0

3.50

3.2  0.7

0

h 1226

h 1223 0

h 1222 2.30  0.70

1.9  1.7

0

0

1.20  0.60

3.0  2.0

h 1212

h 1224

1.70  1.60 0

h 1225

3.20  1.30 0

h 1217

1.90  1.50

7.5  6.1

0

0

h 1207

3.8  0.9 2.10  1.50

h 1204

4.20  3.70 0

h 1209

4.60  1.10 0

h 1205

0

2.00  1.00

3.0  2.4

0

2.20  1.20

6.5  5.9

0

h 1202

h 1200

0

h 1199

1.70  1.60

5.3  1.0

0

0

3.2  1.9

0

0

1.60  1.20

3.2  1.2 h 1197

h 1195

0

5.60  2.60 0

Name/Notes

Size

9, 16, 31

9

28

16, 23

16, 31

1, 4

9, 16, 31

9, 16

28

16

16, 31

16, 31

16, 31

9, 16

9, 16

4, 9

4

9, 16, 31

4

9, 16, 31

9

9, 16, 31

9

23

9, 16, 31

16, 31

9, 16, 31

9, 16, 31

1, 4

9, 16, 31

16, 31

9, 16, 31

9, 16

Map no.

151 4440 4442 4449 4448

H II-173

H II-156 *

H I-213 *

H I-91 *

4438

H I-28.2*

VIR

4434 4435

H II-497

H I-28.1*

VIR

4429 4430

H II-65 *

H II-146

COM

CVN

VIR

VIR

VIR

VIR

VIR

DRA

VIR

VIR

COM

COM

VIR

VIR

VIR

4441

4417

H II-155

4425

4412

H II-34

VIR

COM

H II-848

4413

H II-169

H II-170

4414

H I-77 *

COM VIR

4420

4406/M 86

h 1253

H II-23

4405

H II-88

COM

CVN

4421

4394

H II-55 *

H II-89

4401

H V-29.2

MUS

VIR

4416

4372

h 3390

4419

4388

H II-168

CVN

H II-113 *

4395

H V-29.1

VIR

CVN

COM

CEN

VIR

COM

COM

VIR

h 1260

4387

H II-167

4373

h 3391 4382/M 85

4378

H I-123

4389

4377

H I-12

H II-749

4379

H II-87

h 1242

4374/M 84

h 1237

12 28.2

12 28.2

12 28.1

12 27.9

12 27.8

12 27.7

12 27.5

12 27.4

12 27.4

12 27.3

12 27.2

12 27.0

12 27.0

12 26.9

12 26.8

12 26.8

12 26.6

12 26.5

12 26.4

12 26.2

12 26.1

12 25.9

12 25.9

12 25.8

12 25.8

12 25.8

12 25.7

12 25.6

12 25.4

12 25.3

12 25.3

12 25.2

12 25.2

12 25.1

þ28 37

þ44 06

þ09 48

þ12 18

þ13 01

þ13 05

þ08 09

þ06 15

þ11 07

þ64 48

þ12 44

þ02 30

þ15 28

þ15 03

þ07 56

þ09 35

þ03 58

þ12 37

þ31 13

þ12 57

þ16 11

þ18 13

þ33 31

72 40

þ12 40

þ33 33

þ12 49

þ45 41

þ18 11

39 45

þ04 55

þ14 46

þ15 36

þ12 53

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX/NE

GC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

11.2

9.4

10.4

11.9

10.0

10.8

11.9

11.8

10.2

12.5

11.9

12.0

11.5

11.2

12.3

11.1

12.4

11.9

10.3

8.9

12.2

10.9

–

7.2

11.0

10.0

12.0

12.0

9.1

10.9

11.7

11.7

11.6

9.2

h 1271 h 1270

h 1281 h 1280

3.90  1.40

6.2  4.4

0

h 1279

4.50  1.80 0

h 1276

0

1.8  1.6

the “Eyes”, h 1275

8.50  3.00 0

the “Eyes”, h 1274

3.00  2.20

1.4

0

5.8  2.8

2.30  2.00

h 1278 ¼ h 1291 0

0

3.20  2.50

2.8  1.0

h 1267

h 1263

2.00  1.00 0

h 1264

2.70  2.00 0

h 1262

0

3.30  1.20

1.7  1.5

0

3.30  1.40

1.4  1.2

0

h 1257

h 1259 0

h 1258

4.4  3.0 2.30  1.40

h 1245

0

0

8.90  5.80

1.6  1.1

0

h 1251

0

h 1252

– 3.40  3.20

5.00

5.6  1.5 h 1244

h 1252

13.20  11.00 0

h 1250

1.70  1.10 0

h 1245

0

2.60  1.30

7.1  5.5

0

3.60  2.60

2.9  2.7

0

h 1228

h 1239

0

h 1240

1.70  1.30

2.0  1.6

0

0

6.50  5.60

9

4, 9

16, 31

9, 16, 31

9, 16, 31

9, 16, 31

16, 31

16, 31

9, 16, 31

4

9, 16, 31

16

9, 16, 31

9, 16, 31

16, 31

16, 31

16, 31

9, 16, 31

9

9, 16, 31

9, 16, 31

9, 16

9

28, 30

9, 16, 31

9

9, 16, 31

4, 9

9, 16

23

16, 31

9, 16, 31

9, 16, 31

9, 16, 31

152

COM VIR

CRV VIR

4450 4455 4452 4460 4454 4459 4458 4461 4457 4462

H II-56 *

H II-355

H I-23

H I-212 ¼ H II-750

H II-180

H I-161 *

H II-121

H II-122

H II-35

H III-764

4494 4497

H III-42

4489

H II-91

H I-83 *

4490

H I-198 *

4500

4485

H I-197 *

H I-234

4480

H II-531

4487

4478

H II-124 *

H II-776

4479

H II-116

4492

4463

h 3395

H II-499

VIR

4476

H II-123

4486/M 87

4477

H II-115 *

4488

4474

H II-629

h 1301

4472/M 49

h 1294

H III-484

COM

4473

H II-114 *

VIR

COM

UMA

VIR

VIR

VIR

CVN

CVN

VIR

VIR

COM

MUS

VIR

COM

COM

VIR

COM

VIR

4469 4470

H II-157

H II-18 ¼ H II-19

VIR

VIR

VIR

COM

VIR

CVN

COM

CRU

4439

h 3392

Con

NGC/M

Herschel

12 31.5

12 31.4

12 31.4

12 31.1

12 31.0

12 30.9

12 30.8

12 30.8

12 30.6

12 30.5

12 30.4

12 30.3

12 30.3

12 30.0

12 30.0

12 30.0

12 29.9

12 29.8

12 29.8

12 29.6

12 29.5

12 29.3

12 29.0

12 29.0

12 29.0

12 29.0

12 28.8

12 28.8

12 28.7

12 28.7

12 28.5

12 28.4

þ11 37

þ25 47

þ57 58

08 03

þ08 05

þ08 22

þ12 24

þ16 45

þ41 38

þ41 42

þ04 15

þ12 20

þ13 35

64 48

þ12 21

þ13 38

þ14 04

þ08 00

þ13 26

þ07 49

þ08 45

23 10

þ03 34

þ13 11

þ13 15

þ13 59

01 56

þ44 52

þ11 45

þ22 49

þ17 05

60 06

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

Type

12.5

97

12.3

11.0

12.4

12.1

8.6

11.9

9.5

11.7

12.4

11.4

12.5

7.2

12.0

10.4

11.5

8.3

10.2

12.2

11.5

12.0

10.8

11.1

11.8

10.4

11.9

11.4

11.9

12.4

10.1

8.4

Mag

h 1285

h 1287 h 1290 h 3396

1.9  0.8

0

9, 16, 31

9

h 1307

4.80  3.50 0

4

h 1311

1.60  1.10

16, 31 16

h 1305

1.70  1.60

16, 31

9, 16, 31

9, 16

4, 9

4, 9

4.00  2.80

h 1302

0

h 1303 4.10  1.70

8.3  6.6

0

1.70  1.60

6.4  3.2

0

Cocoon Galaxy, h 1308

h 1306

2.40  1.80 0

h 1299

2.20  1.10

16, 31

9, 16, 31

1.6  1.3

9, 16, 31

28

9, 16, 31

h 1298

h 1296

9, 16, 31

1.80  1.50

0

0

0

6.00

1.8  1.3

0

3.70  3.30

2.4  1.6

9, 16, 31

16, 31 0

10.20  8.30 0

9, 16, 31

4.50  2.50 h 1295

16, 31 16, 31

3.8  1.3 1.30  0.90

23

16

9, 16, 31

9, 16, 31

9, 16, 31

16

4, 9

9, 16, 31

9

9, 16

28

Map no.

0

0

h 1293

h 1286

3.10  1.10

2.6  2.3

0

0

1.6  1.5 3.40  1.40

h 1288

3.50  2.70 0

h 1284

2.30  2.10 0

h 1289

4.20  1.30

2.7  0.6

0

0

h 1282

5.4  4.1 2.60  0.80

Name/Notes

0

0

4.00

Size

153

4531 4535 4532 4536 4545 4539 4540 4548/M 91 4550 4546 4551 4507 4555 4552/M 89 4559

H II-175

H II-500 *

H II-147

H V-2 *

H II-850

h 1338

H II-94 ¼ H II-119

H II-120 *

H I-36 *

H I-160 *

H I-37

h 3399

H II-343

h 1348

H I-92 *

4565

4527

H II-37 *

H V-24 *

4528

H II-67

4553

4534

H II-410

h 3400

4526

H I-38¼H I-31¼H I-119 *

4561

4525

H II-325

H II-407

4519

H II-158

4517

H IV-5 4515

4521

H II-849

4516

4512

h 1321

H III-78

4503

H II-66

h 1324

4498 4501/M 88

H III-69

h 1312

4496

H II-36

COM

CEN

COM

COM

VIR

COM

CEN

VIR

VIR

VIR

COM

COM

COM

DRA

VIR

VIR

VIR

VIR

VIR

VIR

CVN

VIR

COM

VIR

COM

COM

VIR

DRA

DRA

VIR

COM

COM

VIR

12 36.3

12 36.1

12 36.1

12 36.0

12 35.7

12 35.7

12 35.6

12 35.6

12 35.5

12 35.5

12 35.4

12 34.8

12 34.6

12 34.6

12 34.5

12 34.3

12 34.3

12 34.3

12 34.1

12 34.1

12 34.1

12 34.0

12 33.8

12 33.5

12 33.1

12 33.0

12 32.8

12 32.8

12 32.6

12 32.1

12 32.0

12 31.7

12 31.6

þ25 59

39 27

þ19 20

þ27 58

þ12 33

þ26 31

39 55

þ12 16

03 48

þ12 13

þ14 30

þ15 33

þ18 12

þ63 31

þ02 11

þ06 28

þ08 12

þ13 05

þ02 39

þ11 19

þ35 31

þ07 42

þ30 17

þ08 39

þ14 34

þ16 15

þ00 07

þ63 57

þ63 54

þ11 11

þ14 25

þ16 51

þ03 56

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

9.5

12.3

12.4

9.6

9.9

12.4

12.0

12.0

10.3

11.5

10.1

11.8

12.0

12.3

10.3

11.7

9.8

11.7

10.5

11.9

12.4

9.6

12.2

11.6

12.5

12.4

10.5

12.2

12.2

11.1

9.4

11.9

11.2 0

0

0

0

h 1335 h 1345

5.20  4.20

h 1357

9

15.8  2.1

23 0

9, 16 0

h 1355 2.10  1.00

1.50  1.30

9, 16, 31

9 9

h 1352

h 1350

23

10.70  4.40

0

9, 16, 31

16

9, 16, 31

9, 16, 31

9, 16, 31

9, 16

4

16

16, 31

16, 31

9, 16, 31

16

9, 16, 31

9

3.50

1.9  1.4

0

1.60  1.30

1.8  1.4

0

h 1349

h 1339 0

h 1343 3.30  1.60

3.3  0.9

0

0

1.9  1.5

0

0

3.30  1.40

2.5  1.5

0

h 1346

h 1337 0

h 1334

7.60  3.20

2.7  1.2

0

0

7.10  5.00

3.1  2.0

0

h 1333

h 1330

0

h 1331

6.20  2.10

1.6  1.0

0

h 1336

2.60  2.10 0

h 1329

7.00  2.50

16, 31

16, 31 9

h 1328

9, 16, 31

9, 16

16

4

4

9, 16, 31

9, 16, 31

9, 16

16, 31

2.60  1.30

h 1323

h 1326

h 1313

h 1309

3.20  2.50

1.80  0.90

1.4  1.1

0

10.50  1.50

2.5  0.6

0

2.50  0.60

3.5  1.7

0

6.80  3.70

2.9  1.1

0

3.90  3.10

154 4648 4625 4620 4627 4621/M 59 4631 4623

H II-660

h 1387

H II-659

h 1386

H V-42 *

H II-149

4608

H II-69

H I-274

4606

H III-43 4618

4603

h 3406

4612

4597

H II-636

H I-178 ¼ H I-179 *

4594/M 104

H II-148 ¼ H II-20

4605

4592

H II-31

H I-43 *

4586

H I-125

H I-254

4575

h 3403

4596

4580

H I-124

H I-24 *

4579/M 58

h 1368

4595

4578

H II-15

H II-632

HYD

4589

H I-273

4590/M 68

4570

H I-32 *

4593

4571

H III-602

h 3404

4568

H IV-9

H II-183

VIR

4567

H IV-8

VIR

CVN

VIR

CVN

VIR

CVN

DRA

VIR

CVN

VIR

VIR

CEN

VIR

VIR

UMA

VIR

COM

VIR

VIR

CEN

VIR

VIR

VIR

DRA

VIR

COM

VIR

VIR

VIR

4564

H II-68

Con

NGC/M

Herschel

12 42.2

12 42.1

12 42.0

12 42.0

12 42.0

12 41.9

12 41.8

12 41.5

12 41.5

12 41.2

12 41.0

12 40.9

12 40.2

12 40.0

12 40.0

12 39.9

12 39.9

12 39.7

12 39.5

12 39.3

12 38.5

12 37.9

12 37.8

12 37.7

12 37.5

12 37.4

12 36.9

12 36.9

12 36.6

12 36.5

12 36.4

þ07 41

þ32 32

þ11 39

þ32 34

þ12 57

þ41 16

þ74 25

þ07 19

þ41 09

þ10 09

þ11 55

40 59

05 48

11 37

þ61 37

þ10 11

þ15 18

05 21

26 45

00 32

þ04 19

40 32

þ05 22

þ11 49

þ09 33

þ74 12

þ07 15

þ14 13

þ11 14

þ11 15

þ11 26

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

Type

11.9

9.0

9.7

12.0

12.2

12.3

11.9

11.5

10.6

11.0

11.7

12.4

12.0

8.3

10.1

10.5

12.2

11.1

7.3

11.6

11.7

12.3

11.3

9.6

11.2

10.7

10.8

11.2

10.9

11.3

11.0

Mag

0

h 1371 h 1373

5.80  1.50

h 1382 h 1383 h 1385 h 1384

2.70  2.00

h 1392 0

2.20  0.70

15.2  2.8

0

5.40  3.70

1.7  1.0

0

1.80  1.50

h 1387

Humpback Whale Galaxy, h 1397

h 1391

h 1410 1.60  1.40

1.8  1.2

0

0

4.2  3.4

0

0

3.3  1.7

3.30  2.90

16, 31

9

9, 16, 31

9

9, 16, 31

4, 9

1, 4

16, 31

4, 9

16, 31

9, 16, 31

23, 28 0

0

16

16, 23

4

3.40  2.50

Sombrero Galaxy, h 1376

16, 31

4.10  1.90

8.60  4.20

5.9  2.4

0

h 1381

h 1378

4.00  3.00 0

h 1377

1.70  1.10

9, 16, 31

23 16

h 1375

11.0 3.90  2.90

16

16, 31

0

3.8  1.2

0

0

23, 28

16, 31

2.00  1.20

h 1369

16, 31

1, 4

2.10  1.50

h 1365 ¼ h 1366

3.10  2.30

9, 16, 31

h 1374

3.40  2.80

16, 31

9, 16, 31

9, 16, 31

9, 16, 31

9, 16, 31

Map no.

6.00  4.80

h 1361

3.70  1.20

3.6  1.2

0

h 1362 ¼ h 1367

Siamese Twins, h 1359

0

Siamese Twins, h 1358

3.1  2.2 4.60  2.20

h 1356

0

3.50  1.50 0

Name/Notes

Size

155

4660 4658 4665 ¼ 4664 ¼ 4624 4666 4670 4684 4682 4689 4694 4691

H II-71 *

H II-558

H I-142 ¼ H II-39 *

H I-15 *

H III-328

H II-181

H III-523

H II-128 *

H II-72

H II-182

4696

4659

H II-127

h 3424

4650

h 3413

4698

4645

h 3412

4697

4657

H I-177

H I-8 ¼ H III-6 *

4654

H II-126 *

H I-39 *

4656

H I-176 *

VIR

4649/M 60 4653

h 1408

4651

H III-662

COM

4647

CEN

VIR

VIR

VIR

VIR

COM

VIR

VIR

COM

VIR

VIR

VIR

VIR

COM

CEN

CEN

CVN

VIR

CVN

VIR

VIR

VIR

VIR

VIR

VIR

H II-12

H II-38 *

H III-44

4636

H II-70

CEN

4639

4638

h 3409

VIR

4643

4622

H I-14

CRU VIR

H II-125

4632

H II-532

VIR

H I-10 *

4609 4630

h 3407

4624 ¼ 4664

h 1390 ¼ H II-39

12 48.8

12 48.6

12 48.4

12 48.2

12 48.2

12 47.8

12 47.3

12 47.3

12 45.3

12 45.1

12 45.1

12 44.6

12 44.5

12 44.5

12 44.3

12 44.2

12 44.2

12 44.0

12 44.0

12 43.9

12 43.7

12 43.7

12 43.5

12 43.3

12 42.9

12 42.8

12 42.8

12 42.6

12 42.5

12 42.5

12 42.3

12 42.3

41 19

05 48

þ08 29

03 20

þ10 59

þ13 46

10 04

02 43

þ27 08

00 28

þ03 03

10 05

þ11 11

þ13 31

40 44

41 45

þ32 12

þ13 08

þ32 10

00 34

þ11 33

þ16 24

þ11 35

þ01 59

þ13 15

þ02 41

þ11 26

40 45

00 05

þ03 58

62 58

þ03 04

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX/NE

10.2

9.2

10.7

11.1

11.1

10.7

12.4

11.5

12.2

10.8

10.3

12.5

11.2

12.2

11.8

11.8

12.4

10.4

10.1

12.1

8.8

10.6

11.4

10.8

11.4

9.4

11.1

12.5

11.8

12.5

6.9

10.3

h 1396 h 1402 ¼ h 1421 h 1399 ¼ h 1401

5.90  4.60 h 1403 h 1404

3.10  2.50

h 1422 h 1426 h 3423 h 1431

4.30  3.50

4.70  3.30

7.20  4.70

4.0  2.5

0

h 1436

h 1432 0

h 1434 2.70  2.50

3.3  1.6

0

0

2.5  1.2

0

0

1.4  1.2

2.80  1.10

h 1420 0

4.50  1.40 0

h 1419 ¼ h 1390

3.50

2.1  0.9

0

h 3414

h 1417 0

h 1416

1.8  1.3

2.10  1.70

23, 28

16

16, 31

16

9, 16, 31

9, 16, 31

16

16

9

16

16

16

9, 16, 31

9, 16, 31

23, 28 0

0

23, 28

9

3.20  2.70

part of Hockey Stick Galaxy, h 1415

1.30  0.60 2.20  1.40

h 1411

5.00  3.10

9, 16, 31

9

15.3  2.4

16

0

9, 16, 31

9, 16

9, 16, 31

16

9, 16, 31

16

9, 16, 31

23, 28

16

3.10  2.70

7.6  6.2

0

Hockey Stick Galaxy, h 1414

h 1409

0

h 1405

4.00  2.70

2.9  2.3

0

0

2.9  2.0

0

0

2.2  1.4

0

0

1.70  1.60

3.00  1.20

0

28 h 1395

1.70  1.20 16, 31

0

6.0

16

3.50

156 4767

h 3436

4772

H II-24

4775

4771

H II-535

H II-186

4765

H III-544

4779

4751

h 3434

H III-106

4756

H III-281

4785

4762

H II-75 *

4755

4753

H I-16 *

h 3439

4743

h 3435

4754

4739

H III-515

h 3429

4733

H II-73

H I-25 ¼ H II-74 *

4727

H II-298

4746

4731

H I-41

h 1460

4736/M 94

h 1456

4729

4725

H I-84 *

h 3430

4709

h 3428

4747

4750

H IV-78

4742

4713

H I-140

H II-344

4710

H II-95

H I-133

4701 4712

4700

H III-524

H II-578

4699

H I-129 *

h 1442

NGC/M

Herschel

CEN

VIR

VIR

CRU

CEN

VIR

VIR

VIR

CEN

CRV

VIR

VIR

CEN

VIR

VIR

CEN

VIR

COM

VIR

VIR

CRV

VIR

CVN

COM

CEN

DRA

VIR

COM

COM

VIR

VIR

VIR

Con

12 53.9

12 53.8

12 53.8

12 53.6

12 53.5

12 53.5

12 53.4

12 53.2

12 52.9

12 52.9

12 52.9

12 52.4

12 52.3

12 52.3

12 51.9

12 51.8

12 51.8

12 51.8

12 51.6

12 51.1

12 51.0

12 51.0

12 50.9

12 50.4

12 50.1

12 50.1

12 50.0

12 49.6

12 49.6

12 49.2

12 49.1

12 49.0

39 43

06 37

þ09 44

60 20

48 46

þ02 10

þ01 16

þ04 28

42 40

15 25

þ11 14

01 12

41 24

þ11 19

þ12 05

41 08

10 27

þ25 47

08 25

þ10 55

14 20

06 24

þ41 07

þ25 30

41 23

þ72 52

þ05 19

þ15 10

þ25 28

þ03 23

11 25

08 40

RA (2000.0) Dec

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

Type

11.5

11.1

12.2

4.2

12.4

10.7

12.3

12.5

11.2

12.4

10.1

9.9

12.4

10.5

11.9

12.4

11.3

12.2

12.5

11.7

11.9

11.5

8.1

9.3

11.1

11.2

11.4

11.0

12.5

12.1

12.1

9.6

Mag

2.8  2.1

h 1450

0

h 1470

2.20  2.10 2.6  1.2

0

h 1472

2.10  1.80 0

Jewel Box/Kappa Crucis Cluster

10.00

2.0  1.0

0

h 1469

3.40  1.70 0

h 1468

3.80  0.90

23, 28

16

16

28, 29

23, 28

16

16

23, 28 16

h 1467

1.10  0.80

16, 23

9, 16

16

23, 28

9, 16

3.00  1.10

1.7  1.3

0

h 1464

h 1466 0

h 1461

6.0  2.8

8.70  1.70

h 1462 0

0

1.40  0.50

4.4  2.4

0

9, 16 0

23, 28

16, 23

9

16

9, 16

2.10  0.60

h 3432

h 1455

16, 23

16

4, 9

9

23, 28

1, 4

16

9, 16

9

16

16, 23

16

Map no.

1.60

2.60  1.50

3.3  1.3

0

1.40  1.20

2.2

0

h 1453

h 1452

6.6  4.2 1.60  1.20

h 1451

0

0

14.40  12.10

10.7  7.6

0

2.30  2.00

2.1  1.9

0

h 1463

h 1444

0

h 1441

2.90  1.80

4.9  1.2

0

0

2.30  0.90

0

h 1438

3.20  0.80 0

h 1437

3.80  2.80 0

Name/Notes

Size

157 4900 4914 4899

H I-143 *

H II-645

H II-300

4880

H III-83 4877

4852

H II-299

4889

4866

H I-162 *

h 3449

4856

H I-68 *

H II-391

4868

H II-644

4874

4861

H IV-30

4833

4835

h 3448

H II-389

4815

h 3443

h 3444

4832

4831

h 3447 4845 ¼ 4910

4839

H II-386

H II-536 ¼ H V-3 *

4825

H II-563

h 3446

4818

H II-549

4808

H I-141 4804 ¼ 4802

4814

H I-243

4826/M 64

4795

H II-21

H IV-40

4790

H II-560

h 1486

4783 4782

4793

H I-93

H I-136

4800

H I-211 *

H I-135

4781 4786

H I-134 *

H II-187

4789

H II-345

VIR

CVN

VIR

VIR

VIR

CEN

COM

MUS

COM

VIR

VIR

CVN

CVN

CEN

MUS

VIR

CEN

HYD

COM

VIR

VIR

COM

CRV

VIR

UMA

VIR

VIR

CRV

CRV

COM

CVN

VIR

VIR

COM

13 00.9

13 00.7

13 00.6

13 00.4

13 00.2

13 00.1

13 00.1

12 59.6

12 59.6

12 59.5

12 59.3

12 59.1

12 59.0

12 58.1

12 58.0

12 58.0

12 57.8

12 57.6

12 57.4

12 57.2

12 56.8

12 56.7

12 55.9

12 55.8

12 55.4

12 55.0

12 54.9

12 54.6

12 54.6

12 54.6

12 54.6

12 54.5

12 54.4

12 54.3

13 57

þ37 19

þ02 30

15 17

þ12 29

59 36

þ27 58

70 53

þ27 58

þ14 10

15 02

þ37 19

þ34 52

46 15

64 57

þ01 35

39 44

27 18

þ27 30

13 40

08 31

21 41

13 02

þ04 18

þ58 21

þ08 04

10 15

12 34

12 33

þ28 56

þ46 32

06 52

10 32

þ27 04

GX

GX

GX

GX

GX

OC

GX

GC

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

12.2

11.5

11.3

12.4

11.6

8.9

11.5

8.4

11.9

11.1

10.6

12.2

13.5

11.6

8.6

11.3

11.6

12.4

12.0

11.9

11.3

8.5

11.6

11.6

11.7

12.2

12.4

11.7

11.7

11.6

11.6

11.8

11.1

12.1 0

h 1478 h 1475

h 1480

2.80  1.10

0

3.50  2.10

16, 17, 23

9

h 1514

2.20  2.1 2.60  1.40

16, 17, 23 16, 17

h 1509

2.20  1.00

28, 29 9, 16, 17

h 1503

3.10  2.50

9

28, 30

9

9, 16

16, 23

9

9

12.00

2.8  2.0

0

14.00

1.9

0

h 1507

h 1498

0

h 1497 6.40  1.50

4.3  1.2

0

0

1.50  1.40

4.2  1.6

0

23, 28 0

28 h 1499

23, 28 16

4.00  0.90

h 1491

23

5.00

4.90  1.30

1.8  1.2

0

h 1494

9

1.70  0.90

4.00  1.90

16 16, 23

h 1484 ¼ h 3445

4.30  1.50

9

16, 23

16

4

16

2.00  1.10

Blackeye Galaxy

10.00  5.40

2.4  1.6

0

h 1483

3.30  2.40 0

h 1474

2.30  1.60

1.5  0.9

16, 23

16, 23

0

0

16, 23

2.3  1.3 1.80  1.70

9

4, 9

16

16, 23

9

0

0

1.6  1.2 2.90  1.50

h 1473

0

0

1.60  1.30

3.4  1.4

0

1.90  1.50

158 5033

5020

H II-129

5018

5023

H II-664

H I-97 *

5012

H I-85

H II-746

5005

H I-96 *

5024/M 53

4993 ¼ 4994

H III-766

5011

4995

H I-42 *

h 1558

4999

H II-537

h 3473

4984

H II-301

H III-765 4976

4970

h 3466

4981

4965

h 3464

H II-189

4955

H I-130 *

h 3468

4945 4958

h 3459

4947 4946

4951

H II-188

h 3461

4956

H II-413

h 3460

4936 4940

h 3456

4939

H II-561

h 3457

4941

H I-40

4915

H IV-47 4933

4921

H II-393

4930

4902

H I-69

H II-191

4904

H II-517

h 3454

NGC/M

Herschel

CVN

VIR

CEN

COM

VIR

CVN

COM

CVN

HYD

VIR

VIR

VIR

VIR

CEN

HYD

HYD

HYD

VIR

CEN

CEN

CEN

VIR

CVN

CEN

CEN

VIR

VIR

CEN

VIR

VIR

COM

VIR

VIR

Con

13 13.4

13 13.0

13 12.9

13 12.9

13 12.6

13 12.2

13 11.6

13 10.9

13 09.8

13 09.7

13 09.6

13 09.0

13 08.8

13 08.6

13 07.5

13 07.2

13 06.1

13 05.8

13 05.4

13 05.4

13 05.4

13 05.1

13 05.1

13 04.9

13 04.3

13 04.2

13 04.2

13 04.1

13 03.9

13 01.5

13 01.4

13 01.0

13 01.0

þ36 36

19 31

43 06

þ18 10

þ12 36

þ44 02

þ22 55

þ37 03

23 23

07 50

þ01 40

15 31

06 47

49 30

24 02

28 14

29 45

08 01

49 28

43 36

35 20

06 30

þ35 11

47 16

30 32

10 20

05 33

41 24

11 29

04 33

þ27 53

14 31

00 02

RA (2000.0) Dec

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

Type

10.0

10.7

11.3

7.7

12.1

12.1

12.3

9.8

12.4

11.2

12.2

11.3

11.4

10.1

12.2

12.1

12.1

10.7

8.6

12.5

11.9

12.0

12.3

12.4

10.7

11.3

11.2

11.5

12.1

12.1

12.5

10.9

12.1

Mag

2.0  1.1

0

h 3465

h 1556 13.0

0

10.70  5.00

3.4  2.6

0

2.50  2.10

0

h 1564

h 1554

h 1559

5.8  0.8

3.10  2.70

h 1549

2.90  1.70 0

h 1547

5.80  2.90 0

h 3471

1.30  1.10

2.4  1.7

0

h 1540 ¼ h 3472

h 1543

2.30  1.90 0

h 1536

3.60  2.50

9

16, 17, 23

23, 28

9, 16, 17

9, 16, 17

4, 9

9

9

23

16, 17

16, 17

16, 17, 23

23, 28 16, 17

h 1537

5.6  3.0

2.80  1.90

23

1.80  1.00 0

23

2.40  2.00 0

23

1.90  1.30

16, 17

23, 28

3.90  1.40

19.8  4.0

23, 28

23

16, 17

9

0

0

h 1523

23, 28

23

16, 17, 23

16, 17

23, 28

16, 17, 23

16, 17

1.60  1.20

2.4  1.2

0

3.80  1.60

1.5

0

1.00

2.7  2.3

0

h 1525

h 3458

0

h 1520

5.50  2.80

3.9  2.7

0

0

4.40  3.60

0

h 1513

1.60  1.30 0

h 1516

2.40  2.10 9

16, 17 16, 17, 23

h 1511

Map no.

2.00  2.60

Name/Notes

2.20  1.50

Size

159

HYD

5061 5062 5068 5064 5077 5079 5078 5084

H I-138

h 3482

H II-312

h 3483

H II-193

H III-118

H II-566

H II-313

5121 5134

h 3499

h 3498

H II-314

5120

5124

H II-653

5147

5129

h 3495

H II-25

5114

H II-328

h 3496

5127

H IV-70

5135

5144

h 3492

h 3502

5102

H II-646

5128

5112

H II-567

h 3501

5090 5101

h 3487

5085

5045

h 3475

5087

5054

H II-513 *

H II-780

5043

h 3476

H III-724

VIR

5053

H VI-7

HYD

VIR

CEN

HYD

CEN

VIR

CEN

CEN

VIR

CEN

CVN

UMA

CEN

CVN

HYD

CEN

VIR

HYD

VIR

VIR

CEN

VIR

CEN

HYD

CEN

VIR

CEN

COM

CVN

5042

VIR

VIR

5055/M 63

5044

H II-511

h 3477

5037

H II-510

CEN

h 1570

5026

h 3474

13 26.3

13 26.1

13 25.7

13 25.5

13 25.3

13 24.8

13 24.8

13 24.1

13 24.0

13 23.8

13 22.9

13 22.0

13 21.9

13 21.8

13 21.1

13 20.4

13 20.3

13 20.3

13 19.8

13 19.6

13 19.5

13 19.0

13 18.9

13 18.4

13 18.1

13 17.0

13 17.0

13 16.7

13 16.4

13 15.8

13 15.5

13 15.4

13 15.0

13 14.2

þ02 06

63 25

29 50

43 01

21 08

37 41

30 19

þ13 59

32 21

þ31 34

þ70 31

36 38

þ38 44

27 26

43 44

20 37

24 26

21 50

27 24

12 42

12 39

47 55

21 02

35 26

26 50

63 25

16 38

60 04

þ17 42

þ42 02

23 59

16 23

16 35

42 58

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

OC/NE

GC

GX

GX

GX

GX

GX

11.7

10.8

12.0

6.6

11.4

10.7

12.1

12.0

12.5

12.5

12.7

9.5

11.6

10.5

11.5

11.4

11.7

10.5

11.1

12.0

11.4

12.1

9.8

11.6

10.3

–

10.9

–

9.0

8.5

11.8

10.8

12.2

11.6

0

0

0

h 3484 h 1579

0

1.90  1.60

3.0

0

2.60  1.80 h 1601

Black Belt Galaxy/ CEN A

16, 17

28, 29

23

23, 24, 28

2.80  1.70 25.70  20.00

23 23

1.90  1.50 h 1597

23

2.20  0.70

23 9, 16, 17

h 1595

1.70  1.40

9

1, 4

23

4, 9

23

1.80  1.00

2.80  2.20

1.2  0.8

0

h 1596

h 1589

4.00  2.90 8.60  2.70

h 3493

5.40  4.60

2.7  2.2

23, 28

23 0

0

23

3.5  3.0

2.70  2.20

23

23

16, 17, 23

16, 17, 23

23, 28

23

23

23

28, 29

16, 17, 23

28, 29

9, 16, 17

4, 9

23

16, 17, 23

16, 17, 23

23, 28

0

0

4.0  1.9 9.30  1.70

h 1578 ¼ h 3491

h 1577

h 3480

h 1568

0

0

1.50  0.80

2.2  1.6

0

1.90  0.90

7.3  6.4

0

2.30  0.70

3.5  3.0

0

60.00

5.1  2.8

0

0

h 1569

10.00

10.00

h 1566

h 1565

Sunflower Galaxy

0

0

12.60  7.2

4.2  2.2

0

3.00

2.0  0.6

0

3.30  2.10

160 5172 5174 5204 5155 5170 5194/M 51 5195

5198 5182 5168 5188 5193 5218 5189 5206 5230 5220 5236/M 83 5248 5237 5247 5254 5257

H III-45

H IV-63

h 3506

H V-22

h 1622

H I-186 *

H II-689

h 3513

h 3512

h 3515

h 3516

h 1636

h 3514

h 3518

H III-87

h 3521

h 3523

H I-34 *

h 3524

H II-297

h 3527

H II-895

5161

h 3511

h 1613

5156

5152

h 3508

h 3510

5150

h 3507 5153

5138

h 3503

5173

5139

h 3504

H III-672

5140

h 3505

h 3509

NGC/M

Herschel

VIR

VIR

VIR

CEN

BOO

HYD

CEN

VIR

CEN

MUS

UMA

CEN

CEN

CEN

HYD

CVN

CVN

CVN

VIR

CEN

UMA

VIR

COM

CEN

CEN

CVN

HYD

HYD

HYD

CEN

CEN

CEN

Con

13 39.9

13 39.6

13 38.1

13 37.6

13 37.5

13 37.0

13 35.9

13 35.5

13 33.7

13 33.5

13 32.2

13 31.9

13 31.3

13 31.2

13 30.7

13 30.2

13 30.0

13 29.9

13 29.8

13 29.6

13 29.6

13 29.3

13 29.3

13 29.2

13 28.7

13 28.4

13 28.0

13 27.9

13 27.6

13 27.3

13 26.8

13 26.3

þ00 50

11 30

17 53

42 52

þ08 53

29 52

33 28

þ13 40

48 09

65 59

þ62 46

33 14

34 47

60 56

28 08

þ46 40

þ47 16

þ47 12

17 58

63 25

þ58 25

þ11 00

þ17 03

33 10

48 55

þ46 36

29 37

29 37

29 34

59 01

47 29

33 53

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

GX

GX

GX

PN

GX

GX

GX

OC

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GC

GX

Type

12.1

12.4

9.9

12.2

10.1

7.5

12.3

12.3

10.6

10.3p

12.3

11.5

12.1

9.1

12.4

11.7

9.6

8.1

11.4

–

11.1

12.5

11.8

11.4

11.7

12.2

11.9

12.5

11.9

7.6

5.3

11.8

Mag

0

23

4.0

0

1.6  0.8

0

0

3.20  1.50

5.4  4.9

0

2.00  1.60

6.20  4.50

12.9  11.5

0

2.40  0.70

1.9

0

3.80  3.30

2.3

0

1.80  1.30

1.5

0

3.00  1.10

h 1654

h 1649

h 1650

Southern Pinwheel

h 1639

16, 17

16, 17, 23

16, 17, 23

23, 24, 28

9, 16, 17

23

23, 24

9, 16, 17

23, 28

28, 29

4, 5

23

23, 24

28, 29

23 0

4, 9, 10

4, 9

1.90  1.30

companion to Whirlpool Galaxy, h 1623

5.90  4.60

4, 9

16, 17, 23

28, 29

2.00  1.70

Whirlpool Galaxy

h 1612

11.20  6.90

8.2  1.0

0

60.00 0

h 1625

5.00  3.00

4, 5

9, 16, 17 9, 16, 17

h 1612

3.4  1.8 2.70  1.40

23

0

0

23, 28

5.60  2.30

4, 9

2.50  2.00

1.00  0.90

2.0  1.4

0

23

0

1.3  1.0 23

28, 29

23, 28

23

Map no.

2.10  0.70 h 1614

Omega Centauri Cluster

Name/Notes

0

0

8.00

55.0

0

2.10  1.70

Size

161

5308 5292 5303 5300 5288

H I-255

h 3536

H III-681

H II-533

h 3534

5334 5328 5350

H III-665

H III-923

H II-713

5337

5324

H II-307

H III-698

5307

h 3541 5329

5326

H II-712

H III-549

5299 5318

h 3537

H III-423

CVN

HYD

VIR

CVN

VIR

VIR

CEN

CVN

CVN

CVN

UMA

VIR

CVN

CEN

CIR

VIR

CVN

CEN

UMA

BOO

CEN

5293

H V-6

CEN

CEN

CVN

5281

h 3531

5320

5284

h 3532

CEN

5313

5286

h 3533

CVN

H II-669

5297

H I-180

CVN

CVN

H II-711

5301

H II-688

5322

5290

H I-170

CEN

H I-256 *

5269

h 3530

CEN

5306

5266

h 3529

CVN

CVN

H II-306

5272/M 3

h 1663

5302

5273

H I-98 *

HYD

VIR

5311

5264

h 3528

H II-710

5258

H II-896

CEN

h 3539

5253

H II-638

13 53.4

13 52.9

13 52.9

13 52.5

13 52.2

13 52.1

13 51.1

13 50.8

13 50.5

13 50.4

13 50.3

13 49.7

13 49.3

13 49.1

13 49.0

13 48.8

13 48.7

13 48.3

13 47.8

13 47.7

13 47.0

13 46.9

13 46.6

13 46.6

13 46.4

13 46.4

13 46.4

13 45.3

13 44.8

13 43.0

13 42.2

13 42.1

13 41.6

13 40.0

13 39.9

þ40 22

28 29

01 07

þ39 42

þ02 20

06 03

51 12

þ39 34

þ33 43

59 56

þ41 22

þ39 59

þ60 12

07 12

þ40 00

30 31

64 41

þ03 57

þ38 18

30 57

þ60 58

þ16 16

62 54

59 11

51 22

þ43 52

þ46 06

þ41 43

62 55

48 11

þ28 23

þ35 39

29 55

þ00 50

31 39

GX

GX

GX

GX

GX

GX

PN

GX

GX

OC

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

OC

OC/NE

GC

GX

GX

GX

OC/NE

GX

GC

GX

GX

GX

GX

11.6

11.7

11.6

12.5

12.4

11.8

11.2

12.1

12.4

–

12.2

12.1

10.1

12.2

12.5

12.2

11.8

11.8

12.4

12.0

11.4

13.1

5.9

10.0p

7.4

11.7

12.3

12.1

–

11.0

6.3

11.5

12.0

12.1

10.1 0

0

23, 24

h 1677 h 1682

h 1669

3.20  2.30

4, 9, 10

16, 17 23, 24

h 3543

4.2  3.0

1.80  1.20

4, 9, 10

16, 17 0

h 1691 0

h 1686 1.70  0.80

2.30  2.10 1.30

28 16, 17

0.30 h 1681

h 1685

2.20  1.20

4, 9, 10

28, 29 9, 10

h 1679

30.0

1.50  0.90

4, 9, 10

4, 9, 10

4, 5

16, 17

0

1.7  1.0

3.60  1.70

h 1684

6.00  4.10 0

h 1671

1.30  1.00 0

h 1675

2.60  2.30

4, 9, 10

0

1.7  1.0

28, 29

3.00 0

h 1669

3.80  2.40

16, 17

23, 24 4, 9, 10

h 1672

0.90  0.40

4, 5

9, 16, 17

28, 29

28, 29

28

1.80  1.60

3.70  0.70

1.8  1.5

0

8.00

30.0  20.0

0

11.00

h 1674

h 1668

5.60  1.30

4, 9, 10

4, 9, 10 4, 9, 10

h 1670

4.00  0.80

3.7  1.0

0

0

28, 29

0

9, 10 9, 10 23, 28

Spring’s Globular

h 1664

23, 24

16, 17

23, 24

3.00

0

h 1655

h 3526

3.30  2.30

18.00

2.8  2.5

0

2.60  1.50

1.4  0.9

0

5.00  1.90

162 5367 5365 5382 5394 5395 5359 5406 5381 5422 5430 5443 5448 5440 5457/M 101

h 3548

H III-546

H I-191

H I-190

h 3545

H II-699

h 3549

H I-230

H II-827

H II-799

H II-691

H II-416

h 1744

5383

H I-181

h 3547

5375 5380

H II-698

5378

h 1713

h 1711

5377

H I-187

5371

H II-716

5364

5379

H I-239

H II-534 *

5376

H I-238 ¼ H II-844

5363

5362

H II-671

H I-6 *

CEN

5333

h 3544

5357

5345

H II-686

5389

5316

h 3542

h 3546

5351

H II-697

H I-240

CVN

5353

H II-714

UMA

CVN

UMA

UMA

UMA

UMA

CEN

CVN

CIR

CVN

CVN

VIR

CEN

CEN

CVN

CVN

CVN

CVN

CVN

VIR

VIR

UMA

UMA

UMA

CVN

CEN

VIR

CEN

CVN

CVN

CVN

5354

H II-715

Con

NGC/M

Herschel

14 03.2

14 03.0

14 02.8

14 02.2

14 00.8

14 00.7

14 00.6

14 00.3

13 59.8

13 58.6

13 58.6

13 58.2

13 57.9

13 57.7

13 57.1

13 56.9

13 56.8

13 56.8

13 56.3

13 56.2

13 56.1

13 56.1

13 56.0

13 55.7

13 55.6

13 55.3

13 54.9

13 54.5

13 54.3

13 53.9

13 53.5

13 53.5

13 53.5

þ54 21

þ34 46

þ49 10

þ55 49

þ59 20

þ55 10

59 34

þ38 55

70 24

þ37 25

þ37 27

þ06 16

43 57

39 59

þ41 51

þ37 37

þ29 10

þ37 48

þ47 14

þ05 01

þ05 15

þ59 44

30 20

þ40 28

þ59 45

þ59 30

þ41 19

48 31

01 25

62 52

þ37 55

þ40 17

þ40 18

RA (2000.0) Dec

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

DN

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

Type

7.5

12.3

11.2

12.3

12.0

12.0

–

12.3

–

11.7

12.9

12.5

11.4

–

11.5

12.2

12.0

12.5

11.3

10.4

10.5

12.0

12.0

10.5

13.0

12.2

12.4

10.9

12.5

6.0

12.2

11.1

11.5

Mag

0

0

0

2.0

0

h 1738

28.80  26.90

2.2  1.0

0

Pinwheel Galaxy

h 1739

h 1743 0

h 1743 3.80  2.00

2.7  1.0

0

0

3.9  0.7

h 1736

h 1728

h 1723

2.30  1.30

0

0

h 1722

0

0

11.00

1.9  1.4

0

8.00

2.7  1.3

0

1.90  1.30

0.9  0.6

0

3.80  2.10 h 171

h 1717

3.20  2.70 0

h 1714

0

1.70

3.3  2.8

0

2.70  2.20

4.7  2.4

h 1712

h 1705

6.80  4.40 0

h 1703

4.10  2.60 0

h 1719

0

h 1707 ¼ h 1718

h 1693

4.10  1.10

1.6  1.4

0

4.20  3.40

2.2  0.7

0

2.10  1.30

2.2  1.0

0

1.90  1.00

1.6  1.5

0

15.00

2.9  1.6 h 1697

h 1689

2.20  1.10 0

h 1669

1.40  1.30 0

Name/Notes

Size

4, 5

4, 9, 10

4

4, 5

4, 5

4, 5

28, 29

4, 9, 10

28, 29, 30

4, 9, 10

4, 9, 10

16, 17

23, 24, 28

23, 24, 28

4, 9, 10

4, 9, 10

9, 10

4, 9, 10

4, 9, 10

16, 17

16, 17

4, 5

23, 24

4, 9, 10

4, 5

4, 5

4, 9, 10

23, 28

16, 17

28, 29

4, 9, 10

4, 9, 10

4, 9, 10

Map no.

163

5460

h 3555

5546 5557

H II-194

H III-551

H I-99 *

5566

5548

H III-47

H I-144 *

5532

H II-418

5560

5533

h 3562

H II-579

5516

H III-414

5530

5529

H III-134

5585

5523

H IV-49

h 3563

5507

H II-687

H I-235

5494 5506

h 3560

5520

5485

H I-232

H III-676

5481

H II-693

5489

5468

H III-286

h 3559

5480

H II-692

5493

5466

H VI-9 *

H IV-46

5474

H I-214 *

5483

5473

H I-231 *

h 3557

5419

h 3554

5488

5426

H II-309

5490

5427

H II-310

H III-32

5444

H II-417

h 3558

5408

h 3553

VIR

VIR

UMA

LUP

BOO

BOO

BOO

BOO

BOO

CEN

BOO

BOO

VIR

VIR

CEN

BOO

CEN

VIR

CEN

BOO

CEN

CEN

UMA

BOO

VIR

UMA

BOO

UMA

UMA

CEN

VIR

VIR

CVN

CEN

14 20.3

14 20.1

14 19.8

14 18.5

14 18.4

14 18.1

14 18.0

14 16.9

14 16.1

14 15.8

14 15.6

14 14.8

14 13.3

14 13.2

14 12.4

14 12.3

14 12.0

14 11.5

14 10.4

14 10.0

14 08.0

14 07.6

14 07.2

14 06.7

14 06.6

14 06.4

14 05.5

14 05.0

14 04.7

14 03.7

14 03.4

14 03.4

14 03.4

14 03.3

þ03 56

þ04 00

þ56 44

43 24

þ36 30

þ07 34

þ25 08

þ10 48

þ35 21

48 07

þ36 13

þ25 19

03 09

03 13

30 39

þ50 22

46 05

05 03

43 19

þ17 33

33 18

48 19

þ55 00

þ50 43

05 27

þ50 43

þ28 32

þ53 40

þ54 54

33 59

06 04

06 02

þ35 08

41 23

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

GX

10.7

12.4

10.5

11.0

10.9

12.4

12.3

11.9

11.9

12.0

12.1

12.2

12.5

11.9

12.0

12.4

12.2

11.4

11.2

12.0

11.9

5.6

11.3

12.5

12.5

12.3

9.2

10.6

11.4

10.9

12.1

11.4

11.7

11.6

0

0

h 1770 h 1776

2.40  1.90

h 1790 h 1778 h 1779

3.60  0.90 6.60  2.30

4.2  1.8

5.80  3.60

0

0

h 1773 1.30  1.10

1.5  1.2

0

0

h 1766 h 1765

0

1.60

3.1  1.9

0

1.80  1.20

6.0  0.7

h 1764

h 1762

4.70  1.10 0

h 1758

1.60  0.90 0

h 1757

2.70  0.80

2.3  2.1

0

17

17

4, 5

23, 24, 28

4, 9, 10

17

10

10, 17

4, 9, 10

24, 28

4, 9, 10

9, 10

17

17

23, 24

4 0

23, 24, 28

2.00  1.10

1.70  1.50 1.50  1.00

23, 24, 28 17

3.90  3.60 h 1755

23, 24

3.4  1.0

10, 17

h 1752

24, 28

4, 5

4

17

4

9, 10

4

4, 5

2.40  1.90

0

h 1745

h 1746

h 1748

23, 24

17

17

4, 9, 10

23, 24, 28

0

0

35.00

2.3  1.9

0

1.80  1.50

2.4  2.3

0

1.60  1.00

9.0

0

4.70

2.2  1.7

0

4.10  3.30

3.0  1.7

0

h 1734

h 1735

0

h 1741

2.90  2.20

2.5  2.0

0

0

1.90  1.00

164 5662

h 3573

APS

5612 5687

h 3567

H II-808

VIR

5668

H II-574

LUP

CEN

BOO

BOO

5643

BOO

BOO

5676

5669

H II-79

H I-189 *

5665

H II-27

DRA

VIR

BOO

DRA

BOO

VIR

VIR

BOO

CEN

BOO

BOO

UMA

LUP

LIB

LIB

LIB

h 3572

5678

5660

H II-695

H I-237

5638

H II-581

5645

5634

H I-70 *

H II-150

5629

h 1812

5656

5606

h 3568

H II-421

5633

H I-185

5667

5623

H II-329

H II-807

CEN

5631

H I-236 *

5617

5593

h 3566

5653

5605

H III-120

h 3570

5597

H II-330

BOO

5595

BOO

BOO

BOO

VIR

H III-122

5590 ¼ 5580

H III-417

H III-121

5576

H I-146 *

VIR

BOO

5600

5574

H I-145

5614

5582

H II-754

HYA

H II-177

5556

h 3564

Con

H II-420

NGC/M

Herschel

14 35.2

14 34.9

14 34.1

14 33.4

14 32.8

14 32.7

14 32.7

14 32.4

14 32.1

14 30.7

14 30.4

14 30.4

14 30.2

14 29.8

14 29.8

14 29.7

14 29.6

14 28.3

14 27.8

14 27.5

14 27.2

14 26.6

14 25.8

14 25.1

14 24.5

14 24.2

14 24.1

14 23.8

14 21.7

14 21.1

14 20.9

14 20.7

14 20.6

56 33

þ54 29

78 24

þ04 27

þ49 28

44 10

þ09 53

þ08 05

þ57 55

þ07 17

þ35 19

þ59 29

þ31 13

60 43

þ49 37

þ03 14

05 59

þ25 50

59 38

þ46 09

þ33 14

þ56 35

54 49

13 10

16 46

16 43

þ34 52

þ14 38

þ35 11

þ03 16

þ03 14

þ39 42

29 15

RA (2000.0) Dec

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GC

GX

OC

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

Type

5.5

11.7

12.2

11.6

11.1

10.2

11.6

12.0

11.4

12.2

11.9

12.5

12.1

6.3

11.7

11.2

9.5

12.1

7.7

12.2

12.5

11.4

–

12.3

12.0

12.0

11.7

12.0

12.3

10.8

12.2

11.5

11.7

Mag

10.0

1.9  1.1 30.00

2.50  1.90

h 1849

h 1835 0

3.00 0

h 1842

0

h 1833

3.90  1.80

4.7  4.2

0

4.00  2.80

2.1  1.3

0

h 1843

3.30  1.40 0

h 1823

2.60  1.60

28, 29

4, 5

28, 30

17

4, 10

23, 24, 28

10, 17

17

4, 5

17

4, 5 10

h 1829

1.90  1.50

10

28, 29

4

1.70  1.10

1.70  1.30

h 1826

h 1832

2.70  2.60 0

h 1817

2.70  2.40

17

10 17

1.8

h 1813

28, 29

4, 9, 10

5.50

h 1818

0

3.00

2.1  1.1

10

h 1808

1.60  1.10 0

4, 5

h 1820

1.70 0

28, 29

17, 24

17, 24

17, 24

9, 10

10, 17

4, 9, 10

17

17

4, 9, 10

24

Map no.

6.00

1.5  1.3

0

h 1798 ¼ h 3569

h 1793

0

h 1792

2.4  1.3 2.10  1.90

h 1804

h 1797

h 1791 ¼ h 1785

0

0

2.40  2.00

1.4

0

1.80

3.8  2.7

0

h 1783

h 1782

0

h 1786

2.8  1.7 1.50  1.10

Name/Notes 0

0

4.10  3.30

Size

165

5757 5749 5770 5775 5784 5832 5792 5820 5791 5786 5806 5812 5813 5800 5831

H III-690

h 3580

H II-576

H III-554

H II-676

H II-332

H II-683

H II-756

H III-691

h 3583

H II-539

H I-71

H I-127

h 3585

H II-540

5823

5756

h 3581

5845

5750

H I-183

H III-511

5746

H I-126 *

h 3589

5740

H II-538

5838

5715

h 3577

H II-542

5739

H I-171

5822

5728

H I-184

h 3588

5713

H I-182

LUP

5688 5694

h 3575

5701

H II-575

H II-196 *

VIR

5691

H II-681

LUP

VIR

CIR

VIR

LUP

VIR

LUP

VIR

LIB

VIR

CEN

LIB

BOO

LIB

UMI

BOO

VIR

VIR

LUP

LIB

LIB

VIR

VIR

VIR

CIR

BOO

LIB

VIR

HYA

VIR

VIR

5670 5690

h 3574

BOO

5689

H II-582

H I-188 *

15 06.0

15 05.7

15 05.4

15 05.2

15 04.1

15 02.2

15 01.2

15 01.0

15 00.0

14 59.0

14 58.8

14 58.7

14 58.4

14 57.8

14 54.2

14 54.0

14 53.4

14 48.9

14 47.8

14 47.6

14 46.2

14 44.9

14 44.4

14 43.4

14 42.5

14 42.4

14 40.2

14 39.6

14 39.5

14 39.2

14 37.9

14 37.7

14 35.7

14 35.5

þ01 38

55 36

þ02 06

54 21

þ01 13

51 55

þ01 42

07 27

þ01 54

42 01

19 16

þ53 53

01 05

þ71 41

þ42 33

þ03 33

þ03 57

54 31

19 05

14 51

00 13

þ01 57

þ01 41

57 33

þ41 50

17 15

00 17

26 32

45 02

þ05 22

00 24

þ02 17

45 57

þ48 45

GX

OC

GX

OC

GX

OC/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

OC

GX

GX

GX

GC

GX

GX

GX

GX

GX

GX

12.5

7.9

10.9

6.5

11.5

8.0

10.5

11.2

11.7

11.2

11.7

12.3

11.3

12.2

12.4

11.8

12.2

8.8

12.0

12.3

11.6

10.5

11.8

9.8

12.3

11.4

11.0

10.2

11.9

10.9

11.3

12.0

12.0

11.9

h 1889

2.50  1.30

0.70  0.50

12.0

17

28, 29

17

4.20  1.50 0

28, 29

35.00

28, 29 17

h 1899

2.10  1.90

17

17

17

24

17, 24

4, 5

17

1, 4, 5

10

17

17

28, 29

17, 24

17, 24

17

17

17

28, 29

4, 10

17, 24

17

24

23, 24, 28

17

17

17

23, 24, 28

4, 10

5.00

4.0  2.8

0

h 1896

h 3587 0

h 1894 2.30  2.00

3.2  1.6

0

0

2.30  1.20

h 1898

0

h 1887

13.00  1.10

6.8  1.7

0

3.60  2.20

1.9  1.8

0

0

h 1885

1.7  1.3

h 1881

h 1876

4.00  1.10

0

0

0

10.00

2.1  1.7

0

2.80  1.30

3.2  1.5

0

h 1875

h 1874

0

h 1872

7.40  1.30

2.8  1.5

0

0

7.00

2.3  2.1 h 1873

h 1866

3.20  1.90 0

h 1857

2.90  2.50 0

h 3576

3.1  1.9 4.30

0

h 1854

4.30  4.10 0

h 1847

1.90  1.40

h 1848 h 1846

0

3.40  1.00

1.5  0.7

0

3.30  1.00

166 5875 5864 5879 5869 5833 5878 5899 5885 5905 5907 5908 5882 5897 5898 5904/M 5 5903 5915 5921 5928 5930 5925 5949 5927 5936 5937

H II-585

H II-757

H II-545

h 3590

H III-736

H II-650

H III-116

H II-758

H II-759 *

H II-760

h 3594

H VI-8 ¼ H VI-19 *

H III-138

h 1916

H III-139

h 3600

H I-148

H II-874

H II-651

h 3603

H II-906

h 3604

H II-130

H II-401

5854

H II-544 5861

5859

H II-752

H II-755

5843

h 3592

H II-192

5856

H IV-71

5866/M 102

H I-215 * 5850

5846

H I-128 *

H II-543

NGC/M

Herschel

SER

SER

LUP

DRA

NOR

BOO

SER

SER

LIB

LIB

SER

LIB

LIB

LUP

DRA

DRA

DRA

LIB

BOO

LIB

APS

VIR

DRA

VIR

LIB

BOO

VIR

BOO

LUP

BOO

VIR

DRA

VIR

Con

15 30.8

15 30.0

15 28.0

15 28.0

15 27.7

15 26.1

15 25.9

15 21.9

15 21.6

15 18.6

15 18.6

15 18.2

15 17.4

15 16.8

15 16.7

15 15.9

15 15.4

15 15.1

15 15.0

15 13.8

15 11.8

15 09.9

15 09.8

15 09.6

15 09.3

15 09.2

15 07.8

15 07.6

15 07.5

15 07.3

15 07.1

15 06.5

15 06.4

02 49

þ12 59

50 40

þ64 46

54 31

þ41 41

þ18 05

þ05 04

13 06

24 04

þ02 05

24 06

21 01

45 39

þ55 25

þ56 19

þ55 31

10 05

þ42 03

14 16

72 52

þ00 28

þ57 00

þ03 03

11 19

þ52 32

þ02 34

þ19 35

36 20

þ18 27

þ01 33

þ55 46

þ01 36

RA (2000.0) Dec

GX

GX

GC

GX

OC

GX

GX

GX

GX

GX

GC

GX

GC

PN

GX

GX

GX

GX

GX

GX

GX

GX/NE

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

Type

12.3

12.3

8.0

12.1

8.4

12.2

12.5

10.7

12.3

11.2

5.7

11.4

8.4

9.4

12.0

10.4

12.1

11.8

11.8

11.7

12.0

11.9

11.4

11.9

11.6

12.5

11.9

12.5

12.3

6.0p

10.8

9.9

10.1

Mag

h 1902

4.50  3.90

h 1903

h 3597 Hercules cluster rival h 3598

2.70  2.60 23.00 2.70  2.10

0

0

1.90  1.10

1.4  1.3

0

6.00

2.2  1.0

0

20.00

0.9  0.8

0

h 1926 ¼ h 3606

h 1925

h 1923 0

h 1919 2.20  1.60

4.8  4.0

0

0

1.60  1.10

h 3596

11.00

0.3

0

Splinter Galaxy, h 1917

17

10, 17

24, 28, 29

1, 4, 5

28, 29

4, 10

10, 17

17

17, 24

24

17

24

24

24, 29

4, 5

4, 5 3.30  1.40

12.6  1.4

4, 5 0

17

5, 9

17, 24

28, 29, 30

17

4, 5

17

17, 24

4, 5

17

10, 17

24

10, 17

17

4, 5

17

Map no.

4.00  2.60

3.5  3.1

0

h 3595

h 1914 0

h 3593

3.30  1.40

3.5  1.4

0

0

2.10  1.00

2.3  1.6

0

h 1908

h 1910

0

h 1907

4.20  1.30

2.8  0.9

0

0

3.00  1.70

2.3  1.2

0

0

h 1905

2.70  0.80

3.0  0.8

0

0

1.90  1.10

0

h 1909 Formerly thought duplicate of M 101

6.50  3.10

nebulous star, h 1904

h 1901

4.00  3.70

–

Name/Notes

Size

167

5970 5982 5985 5987 5968

H II-76

H II-764 *

H II-766

H II-765

h 3609

h 3618

6093/M 80

6031

h 3616

6067

6025

H II-873

h 3624

6048

h 3615

h 3619

6005

h 1940

6072

6014

H III-973

6070

6068

H II-583

h 3620

6010

H II-657

H III-553

5999 6012

h 3612

6000 6015

H III-739

H VII-29

h 3614

5967 5998

h 3608

5979

5962

H II-96

h 3610

5938

h 3607

5996

5966

H III-634

H II-97

5946

h 3607

5986

5954

H II-179

5990

5953

H II-178

H II-425

5965

H II-762

h 3611

5963

H II-761

SCO

NOR

SCO

SER

NOR

TRA

UMI

NOR

SER

UMI

SER

SER

NOR

DRA

SCO

SCO

APS

TRA

SER

SER

LUP

LUP

DRA

DRA

DRA

SER

SER

TRA

BOO

NOR

SER

SER

DRA

DRA

16 17.0

16 13.2

16 13.0

16 10.0

16 07.6

16 03.7

15 57.6

15 55.8

15 55.8

15 55.4

15 54.4

15 54.2

15 52.2

15 51.4

15 49.9

15 49.4

15 48.1

15 47.7

15 46.9

15 46.4

15 46.1

15 39.9

15 39.9

15 39.6

15 38.7

15 38.5

15 36.5

15 36.4

15 35.8

15 35.5

15 34.6

15 34.5

15 34.0

15 33.5

22 59

54 13

36 14

þ00 43

54 04

60 30

þ70 42

57 26

þ05 57

þ79 00

þ00 32

þ14 35

56 28

þ62 19

29 24

28 36

75 40

61 13

þ17 52

þ02 24

37 47

30 33

þ58 05

þ59 20

þ59 21

þ12 11

þ16 37

66 52

þ39 47

50 40

þ15 12

þ15 12

þ56 42

þ56 35

GC

OC

PN

GX

OC

OC

GX

OC

GX

GX

GX

GX

OC

GX

GX

OC/NE

GX

PN

GX

GX

GC

GX

GX

GX

GX

GX

GX

GX

GX

GC

GX

GX

GX

GX

7.3

5.6

11.7

11.8

8.5

5.1

12.3

10.7

12.5

12.4

12.5

11.9

9.0

11.0

12.2

–

12.0

11.5

12.5

12.3

7.6

12.3

11.9

11.1

11.0

11.5

11.3

10.9

12.3

8.4

12.2

12.0

11.9

12.3

0

0

0

0

0

h 1947

29 Herschel’s Delight

24

15.0

10.00

24, 29

17, 18 0

1.60

3.6  1.8

0

29 0

28, 29, 30

1, 4, 5

28, 29, 30

17

1, 5

17

3.00

0

0

h 1939

10, 17

28, 29, 30

1, 4, 5

24

24

29, 30

28, 29, 30

10, 17

17

24, 29

24

1, 4, 5

1, 4, 5

1, 4, 5

10, 17

10, 17

28, 29, 30

5, 10

24, 29

10, 17

10, 17

1, 4, 5

1, 4, 5

15.00

2.2  1.7

0

5.00

1.7  1.6

0

1.00  0.70

2.0  0.5

0

2.10  1.50

3.0

0

5.40  2.10

1.9  1.6

0

2.00  1.00

2.7  1.7

0

0

h 1938

1.70  0.90 0.30

h 1935

h 1934

h 1928

h 1930

1.60  0.90

9.6

0

2.10  1.90

4.2  1.3

0

5.50  3.00

2.6  1.9

0

3.00  2.00

3.0  2.2

0

2.80  2.50

1.8  1.1

0

0

h 1927, galaxy pair

3.00

1.10  0.50

h 1931 h 1927, galaxy pair

0

1.60  1.30

5.2  0.7

0

3.30  2.60

168 6217 6152 6165 6169 6167 6156 6178 6192 6188 6193 6183 6205/M 13 6207 6200 6210 6204

H I-280 *

h 3631

h 3634

h 3636

h 3635

h 3632

h 3638

h 3641

h 3640

h 3642

h 3639

h 1968

H II-701 *

h 3643

h 1970

h 3644

HER

6173

H III-640 6181

6166

H II-875

6171/M 107

6134

h 3627

H II-753

6139

h 3628

H VI-40 *

HER

6144

H VI-10 *

ARA

HER

ARA

HER

HER

TRA

ARA

ARA

SCO

SCO

TRA

NOR

NOR

NOR

NOR

UMI

OPH

HER

NOR

SCO

SCO

HER

APS

SCO

HER

6101

6124

h 3626 6155

6146

H III-638

NOR

SER

H II-690

6115

h 3625

h 3623

6118

H II-402 *

DRA

NOR

6087 6140

h 3622

H III-740

HER

6106

H II-151

Con

NGC/M

Herschel

16 46.5

16 44.5

16 44.2

16 43.1

16 41.7

16 41.6

16 41.3

16 40.5

16 40.3

16 35.7

16 34.8

16 34.4

16 34.1

16 34.0

16 32.7

16 32.6

16 32.5

16 32.3

16 29.8

16 28.6

16 27.7

16 27.7

16 27.3

16 26.1

16 25.8

16 25.6

16 25.2

16 24.6

16 21.8

16 20.9

16 18.9

16 18.8

47 01

þ23 49

47 29

þ36 50

þ36 28

69 23

48 46

48 47

43 22

45 38

60 36

49 36

44 03

48 06

52 37

þ78 12

13 03

þ19 50

þ40 49

þ39 33

49 09

38 51

26 02

þ48 22

72 12

40 40

þ40 53

51 58

02 17

þ65 23

57 54

þ07 25

RA (2000.0) Dec

OC

PN

OC

GX

GC

GX

OC

DN

OC

OC

GX

OC

OC

PN

OC

GX

GC

GX

GX

GX

OC

GC

GC

GX

GC

OC

GX

OC

GX

GX

OC

GX

Type

8.2

8.8

7.4

11.4

5.8

12.2

5.2

–

8.5

7.2

11.6

6.7

6.6

–

8.1

11.0

7.8

11.8

12.2

11.9

7.2

9.1

9.0

12.4

9.2

5.8

12.5

9.8

11.7

11.2

5.4

12.2

Mag

0

0

0

6.00

24, 29

24, 29 10

¼ Struve 5N

10

0.40

in field with Hercules Cluster, h 1969

3.00  1.20

10

29, 30

24, 29

15.00

Hercules Cluster

0

20.00

1.8  0.6

0

14.00

20.0  12.0

24, 29

24, 29 0

24, 29 5.0

9.00

28, 29, 30

24, 29

24, 29

24, 29

0

1.60  1.40

7.0

0

12.00

2.5  0.5

0

29 0

1, 5 25.00

17, 18, 24

10, 17, 18

5, 10

5, 10

3.00  2.50

13.00

2.5  1.1

0

h 3637

h 1962 0

h 1961

1.9  1.4 1.90  1.40

24, 29 0

0

24, 29

24

5, 10

29, 30

24, 29

5, 10

29

17, 18

6.00

30 NW of Antares, h 3629

0

h 1958

h 1953

1, 4, 5

28, 29, 30

17, 18

Map no.

8.20

7.4

0

1.30  0.90

5.0

0

40.00

1.3  1.0

0

3.40

4.7  1.9

0

6.30  4.60

15.0

h 1952

2.40  1.30 0

Name/Notes

Size

169

6266/M 62 6268 6273/M 19 6284

h 3661

h 3662

h 1975 ¼ h 3663

H VI-11 *

6338 6316 6318 6325

H II-812

H I-45 *

h 3672

h 3676

6304

6259

h 3660

H I-147 *

6256

h 3658

6340

6253

h 3657

H II-767

6250

h 3656

6301

6249

h 3655

H IV-57

6254/M 10

h 1972 ¼ h 3659

6300

6242

h 3654

h 3668

6209

h 3645

6293

6231

h 3652

H VI-12 *

SCO

6235

H II-584 *

6281

6221

h 3649

6287

6227

h 3651

h 3664

6215

h 3647

H II-195 *

OPH

6222

h 3650

ARA

OPH

SCO

OPH

DRA

OPH

DRA

HER

ARA

OPH

OPH

OPH

SCO

OPH

SCO

SCO

ARA

ARA

SCO

OPH

SCO

APS

SCO

OPH

ARA

SCO

ARA

SCO

HER

6208

SCO

OPH

6239

6216

h 3648

H III-727

6218/M 12

h 1971

HER

h 3646

6229

H IV-50 *

17 18.0

17 17.8

17 16.6

17 15.3

17 14.5

17 10.4

17 08.6

17 17.0

17 10.2

17 05.2

17 04.8

17 04.5

17 02.6

17 02.4

17 01.2

17 00.7

16 59.5

16 59.1

16 58.0

16 57.6

16 57.1

16 55.6

16 55.1

16 54.0

16 53.4

16 52.8

16 51.6

16 51.1

16 50.7

16 50.1

16 49.5

16 49.4

16 47.2

16 47.0

23 46

39 27

28 08

þ57 25

29 28

þ72 18

þ42 20

62 49

26 35

22 42

37 54

24 46

26 16

39 44

30 07

44 40

37 07

52 43

45 48

44 47

04 06

39 30

72 32

41 48

22 11

59 13

41 13

58 59

44 45

þ42 44

53 49

44 44

01 57

þ47 32

GC

OC

GC

GX

GC

GX

GX

GX

GC

GC

OC

GC

GC

OC

GC

OC

GC

OC

OC

OC

GC

OC

GX

OC

GC

GX

OC/NE

GX

OC

GX

OC

OC

GC

GC

10.2

11.8

8.1

12.5

8.3

11.0

13.5

10.1

8.3

9.3

5.4

8.9

6.8

9.5

6.4

8.0

11.3

10.2

5.9

8.2

6.6

6.4

11.8

2.6

8.9

10.1

–

11.1

10.1

12.1

7.2

10.1

6.1

9.4

0

0

18.0

5 24 24

24 4.10

h 3671 5.00

5.40

1.5  1.0

0

24

3.00  2.80 0

5, 10 1, 5

1.80  1.10 8.00

29, 30

4.30  2.80 h 1980

h 1977 ¼ h 3667

8.20

24

24 24

8.0

h 3666

24

24

24, 29

4.80

0

24

0

6.20

17.0

6.00

15.0

0

24, 29

24

15.00

4.1

29

24, 29

24, 29

0

0

17, 18

4.00

16.0

6.00

20.0

24, 29 0

29, 30

h 1976 ¼ h 3665

24 24, 29

9.00

Table of SCO Cluster

h 3653

28, 29, 30

24, 29

28, 29, 30

24, 29

5, 10

29

24, 29

17, 18

5, 10

2.00  1.60

14.00

5.0

0

3.50  2.50

0

2.20  2.00

4.0

0

2.40  1.10

18.0

4.00

16.0

4.50

170 6369 6412

H IV-11 *

H VI-41

6425 6440 6437

H I-150 *

h 3704

6392

h 3691

6407

6400

h 3696

h 3703

6397

h 3692

h 3700

SCO

6405/M 6

h 3699

6416

6404

h 4020

6426

6401

H I-44 *

h 3702

6396

h 3693

H II-587 *

APS

6402/M 14

h 1983 ¼ h 3698

SCO

SCO

SGR

SCO

PAV

OPH

SCO

ARA

SCO

SCO

OPH

SCO

OPH

DRA

6388 6434

H III-741

SCO

HER

SCO

ARA

DRA

OPH

SCO

OPH

OPH

SCO

OPH

ARA

SCO

OPH

SCO

ARA

Con

h 3690

6383

6357

h 3682

6389

6355

H I-46 *

h 3689

6356

H I-48 *

H II-901

6337

h 3680

6362

6342

H I-149 *

6374 ¼ 6383

6326

h 3675

h 3687 ¼ h 3689

6334

h 3678

h 3684

6322 6333/M 9

h 1979 ¼ h 3677

6305

h 3669

h 3673

NGC/M

Herschel

17 49.1

17 48.9

17 46.9

17 45.0

17 44.9

17 44.4

17 43.5

17 40.8

17 40.7

17 40.1

17 39.6

17 38.6

17 38.1

17 37.6

17 36.8

17 36.3

17 34.8

17 32.7

17 32.3

17 31.9

17 29.6

17 29.3

17 24.6

17 24.0

17 23.6

17 22.3

17 21.2

17 20.8

17 20.5

17 19.2

17 18.5

17 18.1

35 26

20 22

31 32

60 44

þ03 00

32 21

69 47

36 57

53 40

32 13

33 15

23 55

35 00

03 15

þ72 05

44 44

32 34

þ16 24

32 36

67 03

þ75 42

23 46

34 10

26 21

17 49

38 29

19 35

51 45

35 43

18 31

42 57

59 09

RA (2000.0) Dec

OC/NE

GC

OC

GX

GC

OC

GX

OC

GC

OC

OC

GC

OC

GC

GX

GC

OCþDN

GX

OC

GC

GX

PN

DN

GC

GC

PN

GC

PN

DN

GC

OC

GX

Type

–

9.3

7.2

11.5

10.9

5.7

11.7

8.8

5.3

4.2

10.6

7.4

8.5

7.6

12.4

6.8

5.5

12.1

5.5

8.1

11.6

11.4

–

8.6

8.2

12.3

9.5

12.2p

–

7.8

6.0

12.2

Mag

0

0

10.4

0

0

12.0

0

–

4.4

0

10.00

2.1  1.6

0

4.20

15.0

1.30

0

31.00

33.0

6.00

4.8

0

0

h 1982 ¼ h 3697

Butterfly Cluster

24, 25

24

24, 25

29, 30

18

24, 25

29, 30

24, 25

29

24, 25

24, 25

24

24, 25

1, 5

24, 25, 29

24, 25

10, 18

24

29, 30

1, 5

24

24

24

18, 24

18

h 1987

Little Ghost Nebula, h 1981 ¼ h 3686

Lobster Nebula

h 3681

h 3683

24

18, 14

29

24

18, 24

24, 25, 29

29

Map no.

3.00

0

Name/Notes

11.00

2.30  1.00

0

20.00

2.8  1.9

0

20.00

15.0

0

2.50  2.40

0.60

25.0

4.20

10.0

0.80

4.4

0

0.30

35.0  20.0

0

12.00

5.0

0

1.40  0.80

Size

171

6453 6482 6455 6469 6475/M 7 6500 6501 6494/M 23 6543 6496

h 3708

h 1989

h 3709

h 3711

h 3710

H III-957

H III-958

h 1990

H IV-37 *

h 3715

6531/M 21 6530 6528 6533 6548 6540

H V-9 and H V-13

h 1993

H 3725

H II-200 *

H V-13

H III-555

H II-198 *

6555

6523/M 8

H I-49 *

H II-902

6522

H VII-7 *

6546

6520

h 3714

6544

6492

H IV-41, H V-10, 11 and 12 *

H II-197 *

6514/M 20

H II-199 *

h 3729

6506 6517

h 3717

6483

6451

H VI-13 *

6507

6441

h 3705

H VIII-53

6444

h 3706

h 3713

6445

H II-586 *

HER

SGR

SGR

SGR

HER

SGR

SGR

SGR

SGR

SGR

SGR

SGR

PAV

SGR

OPH

SGR

SGR

PAV

SCO

DRA

SGR

HER

HER

SCO

SGR

SCO

HER

SCO

SCO

SCO

SCO

SGR

18 07.8

18 07.3

18 07.2

18 06.3

18 06.0

18 05.1

18 04.8

18 04.8

18 04.6

18 03.8

18 03.6

18 03.4

18 02.8

18 02.3

18 01.8

17 59.8

17 59.6

17 59.5

17 59.0

17 58.6

17 56.8

17 56.1

17 56.0

17 53.9

17 52.9

17 52.0

17 51.8

17 50.9

17 50.7

17 50.2

17 49.5

17 49.2

þ17 36

25 00

23 20

27 49

þ18 35

24 53

30 03

24 20

22 30

24 23

30 02

27 54

66 25

23 02

08 58

24 39

17 24

63 40

44 16

þ66 38

19 01

þ18 22

þ18 20

34 49

22 21

35 23

þ23 04

34 36

30 13

37 03

34 49

20 01

GX

GC

OC

OC

GX

DN/NE

GC

OC/NE

OC

DN

GC

OC

GX

DN

GC

OC/NE

OC

GX

GC

PN

OC

GX

GX

OC

OC

OC/NE

GX

GC

OC

GC

OC

PN

12.3

7.5

8.0

12.7

11.7

–

9.6

4.6

5.9

5.0p

9.9

7.6

11.8

6.3

10.1

–

9.6

12.0

8.6

8.1

5.5

12.4

12.2

3.3

8.2

–

11.3

10.2

8.2

7.2

–

11.2

0

10, 11

0

2.10  1.70

9.20

15.0

h 1994

11, 18

24, 25

24, 25

24, 25 0

10, 11, 18

24, 25 1.50

part of Lagoon Nebula

24, 25 2.90  2.80

–

h 3723

in Lagoon Nebula

24, 25 5.00

15.0

24, 25 0

24, 25

24, 25

24, 25

29, 30

24, 25

16.00

45.0

Lagoon Nebula, h 3722

h 3720 0

h 3721

5.0

9.40

Trifid Nebula, h 1991

0

2.50  1.20

20.0

18 0

24, 25 h 3719

18, 24, 25

29, 30

24, 25, 29

1, 5

18, 24, 25

10, 11, 18

10, 11, 18

–

0

0

4.00

7.00

1.6  0.9

0

5.60

0.3

0

25.00

1.8  1.6

0

2.20  1.60

Cat’s Eye/Snail Nebula

24, 25

75.00

24, 25

0

8.0

24, 25

1.00

2.1  1.8

24, 25

7.60

Ptolemy’s Cluster

h 3707

8.00 24, 25

24, 25 24, 25

3rd mag. G SCO in field

18, 24

9.60

Little Gem Nebula, h 1986

12.00

0.70

172 6595 6605 6596 6604 6603 6584 6611/M 16 6613/M 18 6618/M 17

6438 6625 6624 6626/M 28 6629 6631 6633 6639 6638 6637/M 69

h 2002

h 2005

H VIII-55

H VIII-15

h 2004

h 3737

h 2006

h 2007

h 2008

h 3701

h 2009

H I-50 *

h 2010 ¼ h 3743

H II-204 *

h 3746

H VIII-72 *

h 2011

H I-51 *

h 3747

6568

H VII-30 *

6583

6572

h 2000

H VII-31 *

6563

h 3734

6569

6561

H VIII-54

6573

6558

h 3731

H II-201 *

6559

h 1996 ¼ h 3733

h 1999

6554 6553

H IV-12 *

6541

h 3726

h 1995

NGC/M

Herschel

SGR

SGR

SCT

OPH

SCT

SGR

SGR

SGR

SCT

OCT

SGR

SGR

SER

TEL

SGR

SER

SGR

SER

SGR

SGR

SGR

SGR

SGR

OPH

SGR

SGR

SGR

SGR

SGR

SGR

CRA

Con

18 31.4

18 30.9

18 30.1

18 27.7

18 27.2

18 25.7

18 24.5

18 23.7

18 23.2

18 22.3

18 20.8

18 19.9

18 18.8

18 18.6

18 18.4

18 18.1

18 17.5

18 17.1

18 17.0

18 15.8

18 13.8

18 13.6

18 12.8

18 12.1

18 12.0

18 10.5

18 10.3

18 10.0

18 09.3

18 09.1

18 08.0

32 21

25 30

13 12

þ06 34

12 02

23 12

24 52

30 22

12 03

85 24

16 11

17 08

13 47

52 13

18 25

12 14

16 40

14 58

19 53

22 08

22 10

31 50

21 36

þ06 51

33 52

16 48

31 46

24 06

25 54

18 26

43 42

RA (2000.0) Dec

GC

GC

OC

OC

OC

PN

GC

GC

OC

GX

DN

OC

DNþOC

GC

OC

OC

OC

OC

OC

OC

OC/NE

GC

OC

PN

PN

OC/NE

GC

DN

GC

OC/NE

GC

Type

8.3

9.2

–

4.6

11.7

11.3

6.9

7.6

9.0

11.7

6.0

6.9

6.0

7.9

11.1

6.5

–

6.0

7.0

10.0

–

8.4

8.6

8.1

11.0

–

8.6

–

8.3

–

6.3

Mag

0

h 1997

–

6.0

0

25

25 7.10

h 3748

18 7.30

CH 8

18, 25

25

18, 25

0

h 3744

25

25

–

20.0

7.00

0.3

0

13.80

8.8

h 3742

18, 25 0

30

18, 25

18, 25

18, 25

29

18, 25

18, 25

39.00

Omega/Horseshoe/ Swan/Checkmark Nebula

Eagle Nebula/Cluster

in M 24/SGR MW Star Cloud

1.60  1.40

20.0  15.0

7.00

8.0

0

6.60

4.00

h 3740

18, 25

10.00 0

18, 25

29.00

25 18, 25

h 2001 ¼ h 3739

11.00

5.00

24, 25

25

18

25

h 3736

h 1998 ¼ h 3735

24, 25

18, 25

–

6.4

0

12.00

0.2

0

0.80 ¼ Struve 6N

24, 25

4.20

24, 25

24, 25

0

8.0  5.0

18, 25

24, 25, 29

Map no.

9.20 0

Name/Notes

–

15.00

Size

173 6737 6749

h 2026

h 2029

6721

h 3767 6738

6735

h 2025 6743

6728

H VIII-13

h 2027

6723

h 2028

6724

6717

H III-143

h 3770

6716

h 2021

h 2024

6720/M 57

h 2023

6715/M 54

6712

H I-47 *

6708

6699

h 3759

h 3763

6709

h 2020

h 4021

6705/M 11

h 2019

6673

h 3755

6684

6653

h 3750

h 3757

6681/M 70

h 3756

6694/M 26

6683

h 2018

6698

6682

h 2017

H VI-15

6664

H VIII-12 *

h 3758

6652 6656/M 22

6659

h 2016

h 2015 ¼ h 3753

6649

h 3751

h 3752

6642 6645

H II-205 *

H VI-23 *

6647

H VIII-14

AQL

SGR

AQL

LYR

PAV

AQL

AQL

SGR

AQL

TEL

SGR

SGR

SGR

LYR

SCT

PAV

AQL

SCT

PAV

SGR

SCT

PAV

PAV

SGR

SCT

SCT

SCT

SGR

SGR

HER

SCT

SGR

SGR

SGR

19 05.4

19 02.2

19 01.4

19 01.4

19 00.8

19 00.8

19 00.0

18 59.6

18 57.0

18 55.6

18 55.1

18 55.1

18 54.6

18 53.6

18 53.1

18 52.1

18 51.5

18 51.1

18 49.0

18 48.2

18 45.2

18 45.1

18 44.6

18 43.2

18 42.2

18 41.6

18 36.7

18 36.4

18 35.8

18 33.9

18 33.5

18 32.6

18 31.9

18 31.5

þ01 54

18 32

þ11 36

þ29 16

57 47

00 28

08 57

36 38

þ10 22

53 43

30 29

22 42

19 53

þ33 02

08 42

57 19

þ10 21

06 16

65 11

25 55

09 24

62 17

73 16

32 18

06 17

04 46

08 13

23 54

32 59

þ23 34

10 24

16 54

23 29

17 21

GC

OC/NE

OC

OC/NE

GX

OC

OC/NE

GC

OC/NE

GX

GC

GC

OC

PN

GC

GX

OC

OC

GX

OC/NE

OC

GX

GX

GC

OC

OC/NE

OC

GC

GC

OC/NE

OC

OC

GC

OC

12.4

–

8.3

–

12.1

–

–

6.8

–

12.0

7.7

8.4

7.5

8.8

8.1

11.9

6.7

5.8

10.3

–

8.0

11.6

12.5

7.8

9.4

–

7.8

5.2

8.5

–

8.9

8.5

8.9

8.0p 0

29, 30 18, 25

0

Wild Duck Cluster

29, 30

25 29

18, 19, 25 18, 19

–

11, 18, 19 4.00

11 15.00

29

1.60  1.40 –

18, 19

–

18, 19

25

13.00 –

11, 18

–

12.0

1.20  0.90

25 0

18, 25 h 2022 ¼ h 3766

5.40

11 10.00

Ring Nebula

18 3.00  2.40

h 3762

29 0

9.8

11, 18

11.00 1.50

29, 30 18

4.60  2.90 15.00

25

–

10.0

1.7  1.5 2.20  1.00

25 0

8.00 0

18

3.00

18 18

h 3754

12.00

25

–

Hercules Cluster Rival

32.00

6.0

25

11

0

18, 25

18, 25

25

18, 25

7.00  5.00

h 2013

h 2012 ¼ h 3749

h 2014

6.00

15.00

5.8

–

174 6775 6781 6769 6785 6793 6782 6776 6795 6788 6800 6802 6804 6811 6809/M 55 6815 6819 6814 6823 6810

H III-743 *

h 3783

h 2038

H VIII-81

h 3789

h 3787

h 2040

h 3791

H VIII-21

H VI-14 *

H VI-38

h 2044

h 3798

h 2046

h 2048

H III-744

H VII-18 *

h 3797

6774

h 2034

h 2035

6779/M 56

h 2036

6753

h 3779

6768

6754

h 3780

6773

6752

h 3778

h 3786

6744

h 3776

h 2033

6756

H VII-62 *

6758

6739

h 3775

6772

6755

H VII-19 *

H IV-14

6730

h 3771

h 3781

NGC/M

Herschel

PAV

VUL

AQL

CYG

VUL

SGR

CYG

AQL

VUL

VUL

TEL

AQL

PAV

PAV

VUL

AQL

PAV

AQL

AQL

SGR

LYR

CRA

AQL

AQL

TEL

PAV

TEL

PAV

PAV

AQL

PAV

AQL

PAV

Con

19 43.6

19 43.1

19 42.7

19 41.3

19 40.9

19 40.0

19 37.3

19 31.6

19 30.6

19 27.2

19 26.9

19 26.1

19 25.4

19 24.0

19 23.2

19 18.5

19 18.4

19 18.4

19 16.8

19 16.6

19 16.6

19 16.5

19 15.0

19 14.6

19 13.9

19 11.4

19 11.4

19 10.9

19 09.8

19 08.7

19 07.8

19 07.8

19 07.6

58 40

þ23 18

10 19

þ40 11

þ26 51

30 58

þ46 23

þ09 13

þ20 16

þ25 08

54 57

þ03 31

63 52

59 55

þ22 11

01 36

60 31

þ06 33

00 55

16 16

þ30 11

40 11

þ04 53

02 42

56 19

57 03

50 39

59 59

63 51

þ04 41

61 22

þ04 14

68 55

RA (2000.0) Dec

GX

OC

GX

OC

OC

GC

OC

PN

OC

OC

GX

OC/NE

GX

GX

OC

PN

GX

PN

OC

OC

GC

GX

OC/NE

PN

GX

GX

GX

GC

GX

OC

GX

OC

GX

Type

11.6

7.1

11.3

7.3

–

6.3

6.8

12.0

8.8

–

12.1

–

12.1

11.0

–

12.3

11.6

11.4

–

–

8.4

12.2

–

12.7

11.6

11.1

12.1

5.3

8.3

10.6

12.1

7.5

11.3

Mag

8.8

h 2041 h 2042 h 2043

0

7.0

1.20  0.90

h 2049

26, 29, 30

11

18, 19

h 2045

3.00  2.80 0

5, 11

Foxhead Cluster, CH 16

5.00

25 11

19.0

5, 11

18, 19

11, 18, 19

11

–

0

15.00

1.1

5.0

5.00

29 0

18, 19

–

26, 29, 30

1.60  1.40 2.90  0.90

26, 29, 30

2.40  2.00

18, 19 11

h 2039

26, 29, 30

18, 19

7.00

0

18, 19

26, 29, 30

0.60

2.2  1.5

0

1.90

–

20.00

11

25, 29

0

18, 19

–

small asterism

29 18, 19

1.20  1.10

1.40

2.3  1.7 h 2032

29

0

2.40  2.10 0

25, 29

1.80  0.90

26, 29, 30 26, 29, 30

29.00 Pavo Globular Cluster

20.10  12.90

26, 29, 30 18, 19

4.00 h 2031

2.40  0.90

29, 30 18, 19

h 2030

Map no.

15.00

Name/Notes

1.80  1.50

Size

175

6838/M 71

h 2056

6864/M 75

h 2064

6873

6871

h 2067

h 2068

6854

h 3808

6861

6863

h 2065

6874

6866

H VII-59 *

H VIII-86

6851

h 3807

h 3811

6858

h 2061

H III-144 6849

6857

h 2060

6848

6853/M 27

h 2063

h 3805

6856

H II-202

h 3804

6843 6847

h 2059

6839

6837

H VIII-18

6840

6834

H VIII-16 *

H VIII-19

6830

H VII-9 *

H VI-16

6832 6828

H IV-73 *

H VIII-73

6826

H IV-51 *

h 2053

6808 6818

h 3794

6824

H II-878

SGE

CYG

TEL

SGR

CYG

TEL

AQL

CYG

TEL

AQL

TEL

SGR

CYG

VUL

CYG

VUL

AQL

AQL

SGE

SGE

AQL

CYG

VUL

AQL

DRA

CYG

SGR

PAV

CYG

20 08.3

20 07.8

20 07.3

20 06.1

20 05.9

20 05.7

20 05.1

20 03.7

20 03.6

20 03.1

20 02.8

20 06.2

20 01.9

19 59.6

19 59.3

19 57.0

19 56.1

19 55.3

19 54.5

19 53.8

19 53.5

19 52.2

19 51.0

19 50.4

19 48.1

19 44.8

19 44.0

19 43.9

19 43.7

þ21 06

þ38 14

48 22

21 55

þ35 47

54 23

03 34

þ44 00

48 17

þ11 16

56 05

40 12

þ33 31

þ22 43

þ56 08

þ29 20

þ12 09

þ12 06

þ17 54

þ18 47

þ11 41

þ29 25

þ23 04

þ07 55

þ59 25

þ50 31

14 09

70 39

þ56 07

OC

OC/NE

GX

GC

OC

GX

OC

OC

GX

OC/NE

GX

GX

PN

PN

OC/NE

OCþDN/ NE

OC

OC

OC/NE

GC

OC

OC

OC

OC/NE

OC/NE

PN

PN

GX

GX

–

–

11.1

8.6

5.2

12.3

–

7.6

11.7

–

11.6

12.0

11.4p

7.4

–

–

–

–

–

8.4

12.0

7.8

7.9

–

–

8.8

9.3

11.6

12.2

h 2054 h 2055

6.00 0

6.7

–

–

3.0  2.0

0

0

includes Struve 2631

h 2069

includes Struve 2630

11

5, 11

25, 29

25

5, 11 6.80

30.0

26, 29

19

5, 11

0

small starchain asterism

Kite Cluster, CH 7, h 2066

25, 29

11, 19

26, 29, 30

25, 29

11

11

2.00  1.30

–

7.0

0

2.00  1.50

5.0

0

2.40  1.00

1.9  1.1

0

0.60

h 2062

1, 2, 5 0

3.00

11, 18, 19

11, 18, 19

11, 18, 19

11

Dumbbell Nebula

h 2058

11, 18, 19

11, 18, 19

11

11

18, 19

1, 2, 5

5, 11

18, 19, 25

26, 29, 30

5

–

–

–

–

7.20 h 2057

h 2052

6.00 3.0

h 2051

–

0

Blinking Planetary, h 2050

0.60 –

Little Gem Nebula, h 2047

0

0.80

1.6  0.9

0

1.90  1.40

176 CYG SGR

6903 6913/M 29

6946

H IV-76 *

MIC

6934

H I-103 * 6925

6926

H III-142

6940

6923

h 3832

h 3834

6939

H VI-42 *

H VII-8 *

DEL

6909

h 3828

CEP

VUL

AQL

MIC

CEP

TEL

CAP

6902 6907

h 3827

H III-141

CAP

CYG

DEL

VUL

TEL

PAV

h 2073

6893

h 3825

h 2078

6880

h 3820

PAV

6910

6877

h 3818

PAV

H VIII-56 *

6876

h 3817

SGR

TEL

6904

6890

h 3824

6905

6887

h 3822

PAV

H IV-16 *

6872

h 3816

CYG

CYG

CYG

h 2074

6894

H IV-13

TEL

6875 6895

h 3819

H VIII-20 *

H VIII-83

VUL

6888 6885

H IV-72

CYG VUL

6883

TEL

6882

6870

h 3815

TEL

H VIII-22 *

6868

h 3814

Con

h 2070

NGC/M

Herschel

20 34.8

20 34.6

20 34.3

20 34.2

20 33.1

20 31.7

20 31.4

20 27.7

20 25.1

20 24.5

20 23.9

20 23.6

20 23.1

20 22.4

20 21.8

20 20.8

20 19.5

20 18.6

20 18.3

20 18.3

20 17.2

20 16.9

20 16.4

20 16.4

20 13.2

20 12.0

20 12.0

20 11.7

20 11.3

20 10.2

20 09.9

þ60 09

þ28 18

31 59

þ07 24

02 01

30 50

þ60 38

47 02

24 49

43 39

þ38 32

19 19

þ40 47

þ20 07

þ25 45

48 14

70 52

70 51

70 52

44 48

52 47

70 46

þ30 34

þ50 14

46 09

þ26 29

þ38 21

þ26 33

þ35 51

48 17

48 23

RA (2000.0) Dec

GX

OC

GX

GC

GX

GX

OC

GX

GX

GX

OC

GX

OC

PN

OC/NE

GX

GX

GX

GX

GX

GX

GX

PN

OC/NE

GX

OC

DN

OC

OC

GX

GX

Type

9.0

6.3

11.3

8.9

12.5

11.9

7.8

11.6

11.1

10.9

6.6

11.9

7.4

11.1

–

11.7

12.3

12.2

10.7

12.2

12.0

11.7

12.3

–

12.0

8.1

10.0p

8.1

8.0

12.4

10.6

Mag

0

h 2072

26, 29, 30

1.10  0.60

0

0

0

11.5  9.8

0

25.00

4.4  1.1

0

7.10

2.0  1.4

0

h 2084, in field with H VI-42

h 2081

h 2079

1, 2, 5

11

25

19

19

25

1, 2, 5 2.60  1.30

25, 29 h 2083, in field with H IV-76

25, 29 25 10.00

h 2076

5, 11

19, 25

5, 11

11, 19

11

25, 29

2.20  1.10

3.40  2.60

5.6  3.9

0

10.00

1.5

CH 6

h 2077

10.00 0

Blue Flash Nebula, h 2075

1.20

3.0

0

2.60  1.70

2.0  0.9

0

26, 29, 30

26, 29, 30

2.70  2.40 0

26, 29 25, 29

1.60  1.3’

3.2  1.3

0

0

26, 29, 30

11

6.00  1.50

0.90

25, 29

11

5, 11

5, 11

0

h 2071

Crescent Nebula

–

2.4  1.4

0

20.00

18.0  13.0

0

20.00 11

5, 11 0

25, 29

0

35.0

25, 29

Map no.

2.60  1.30

Name/Notes

3.60  2.80

Size

177

6970 6981/M 72 6989 6996 6992 6997 6991 6995 6984 6987 7000 7023 7008 7006 7011 7013 7002 7009

h 3842

h 2090

H VIII-82

h 2094

H V-14

H VIII-58

H VIII-76

h 2093

h 3845

h 3846

H V-37 *

H IV-74

H I-192 *

H I-52 *

h 2101

H II-203

h 3848

H IV-1 *

MIC

6958 6979

6962

H II-426

h 3841

6960

H V-15

H II-206

AQR

6943

h 3838

OCT

AQR

IND

CYG

CYG

DEL

CYG

CEP

CYG

IND

IND

CYG

CYG

CYG

CYG

CYG

CYG

AQR

IND

CYG

CYG

PAV

DEL

6920

PAV

DEL

6956

6932

h 3833

H III-219

6950

H VIII-23

IND

IND

VUL

h 3829

6935 6942

h 3835

h 3837

6938

H VIII-17

21 04.2

21 03.6

21 03.6

21 01.9

21 01.5

21 00.6

21 00.5

20 58.8

20 58.0

20 57.9

20 57.1

20 56.6

20 56.5

20 56.4

20 56.4

20 54.1

20 53.5

20 52.1

20 51.0

20 48.6

20 47.3

20 45.7

20 44.5

20 44.0

20 43.9

20 42.1

20 41.2

20 40.8

20 38.4

20 34.8

11 22

49 01

þ29 54

þ49 19

þ16 11

þ54 33

þ68 10

þ44 20

48 37

51 52

þ31 13

þ47 25

þ44 38

þ31 43

þ45 28

þ45 17

12 32

48 48

þ32 09

38 00

þ00 19

þ30 43

68 45

þ12 31

80 00

73 37

þ16 38

54 19

52 06

þ22 15

PN

GX

GX

OC/NE

GC

PN

DNþOC

DN

GX

GX

SR

OC

OC

SR

OC

OC/NE

GC

GX

SR

GX

GX

SR

GX

GX

GX

GX

OC/NE

GX

GX

OC/NE

8.0

12.4

11.5

–

10.6

10.7

7.1p

4.0p

12.5

12.5

7.0

–

10.0

7.0

10.0

–

9.2

12.3

–

11.3

12.2

7.0

11.3

12.4

11.5

12.4

–

11.7

11.9

–

5.0 30

19, 25

6.60

0.6

0

1.50  1.20 Saturn Nebula, h 2098, ¼ Struve 8N

h 2102

h 2097

3.60 4.00  1.40

h 2099

1.40

Mini-Hyades Cluster

Iris Nebula

10.00  8.00

–

North America Nebula, h 2096

120.0  100.00

0

19, 25

25, 26, 29

11

2, 5, 11

11, 19

2, 5

1, 2, 5

5, 11

25, 26, 29

11

5, 11

26, 29

part of Veil/Filamentary/ Cirrus Nebula, h 2093

h 2091

5, 11

1.40  1.20

0

in North America Nebula

1.80  1.20

12.0

–

8.00

11

5, 11

60.0  8.0

5, 11

– 5.00 0

25, 26, 29

1.00  0.60

part of Veil/Filamentary/ Cirrus Nebula, h 2092

11

0

25

7.00  3.00

2.5  1.9

0

part of Veil/Filamentary/ Cirrus Nebula

h 2087

2.90  2.20

19

11

0

26, 29, 30

11, 19

Veil/Filamentary/Cirrus Nebula, h 2088

h 2086

26, 29, 30

70.00  0.60

0

11, 19

4.00  2.20

1.90

1.8  1.5

0

2.20  1.60

h 2085

26, 29

0

2.1  1.8 26, 29

11

2.10  1.60

h 2082 0

0

8.00

178 7067

H VII-50

7084 7092/M 39 7079 7089/M 2 7093 7083 7090

h 2123

h 2126

h 3869

h 2125

h 2127

h 3870

h 3872

7070

7062

H VII-51 *

7086

7058

h 2115

h 3866

7055

h 2114

H VI-32 *

7049

h 3860

7078/M 15

7041

h 3859

7082

7038

h 3858

h 2120

7050

h 2111

H VII-52

7042

H III-209

7059

7044

H VI-24 *

h 3862

7029

h 3856

7063

7020 ¼ 7021

h 3853 ¼ h 3854

7071

7039

h 2107

h 2117

7037

h 2106

h 2119

7014

7031

H VIII-74 7036

7024

H VIII-57

h 3852

7007

h 3850

h 2104

NGC/M

Herschel

IND

IND

CYG

AQR

GRU

CYG

PEG

GRU

CYG

PEG

CYG

PAV

CYG

CYG

CYG

CYG

CYG

CEP

IND

IND

IND

CYG

PEG

OC

IND

PAV

CYG

CYG

PEG

IND

CYG

CYG

IND

Con

21 36.5

21 35.7

21 34.8

21 33.5

21 32.5

21 32.2

21 31.8

21 30.5

21 30.5

21 30.0

21 29.4

21 27.4

21 26.5

21 24.4

21 24.2

21 23.2

21 21.0

21 19.4

21 19.0

21 16.5

21 15.2

21 15.1

21 13.8

21 12.9

21 11.9

21 11.4

21 11.2

21 10.7

21 10.2

21 07.9

21 07.3

21 06.0

21 05.5

54 33

63 54

þ46 01

00 49

44 05

þ48 26

þ17 25

43 06

þ51 35

þ12 10

þ47 05

60 01

þ47 57

þ36 30

þ48 01

þ46 23

þ50 48

þ57 35

48 34

48 22

47 13

þ36 12

þ13 33

þ42 29

49 17

64 03

þ45 39

þ33 43

þ15 27

47 11

þ50 50

þ41 30

52 33

RA (2000.0) Dec

GX

GX

OC/NE

GC

GX

OC

OC

GX

OC

GC

OC

GX

OC/NE

OC

OC

OC

OC/NE

OC/NE

GX

GX

GX

OC/NE

GX

OC

GX

GX

OC

OC/NE

OC/NE

GX

OC

OC/NE

GX

Type

10.7

11.1

–

6.6

11.5

4.6

–

12.1

8.4

6.3

7.2

11.8

–

7.0

9.7

8.3

–

–

10.6

11.1

12.0

–

12.0

12.0

11.4

11.8

7.6

–

–

12.3

9.1

–

11.9

Mag

h 2110

25, 26, 29

25, 26

9.0

12.0 20.0

7.3  1.2

0

26, 29

26, 29 0

2, 6, 11

19

20, 25, 26

2, 11

11, 19

20, 25, 26

2, 5

–

0

¼ Struve 9N

h 2124

3.90  2.30

16.00

2.0  1.2

0

31.00

0

2.40  1.90

0

11, 19

2, 11 18.00

24.0

26, 29 0

h 2122

11 2, 11 3.30  1.70

–

trapezium/star chain asterism

h 2118

3.00

2, 11

2, 11

h 2116

5.00 0

2, 5

–

4.0

0

2, 5

25, 26

3.6  1.5 4.50  3.00

25, 26

0

0

11

–

11, 19

3.10  1.40

2.00  1.80

7.0

0

2, 11

26, 29, 30

3.5  1.6 2.50  1.40

2, 11 0

0

11

15.00

11, 19

25, 26, 29

2, 5

11

26, 29

Map no.

–

–

1.7  1.4

0

h 2105

0

h 2103

15.00

Name/Notes

–

2.00  1.20

Size

179

7154 7175 7167 7177 7166 7171 7172 7173 7176 7168 7183

h 2141

h 3905

H II-247

h 3903

H III-692

h 3908

h 3909

h 3911

h 3904

H II-595

7156

H III-452 7155

7160

H VIII-67 *

h 3900

7145

h 3895

h 3899

7144

h 3894

7135

h 3891 7123

7125

h 3887

7140 ¼ 7141

7126

h 3889

h 3892 ¼ h 3893

7130

h 3890

h 3886

7124

7118

h 3884 7137

7142

H VII-66 *

H II-261

7098

h 3876

h 3888

7127

h 3874 7128

7096

H IV-75

H VII-40 *

7129

h 2128 ¼ h 3878

h 2129

7097 7099/M 30

h 3877

7095

h 3875

AQR

IND

PSA

PSA

PSA

AQR

GRU

PEG

AQR

CYG

IND

PSA

PEG

CEP

GRU

GRU

IND

IND

PSA

IND

IND

PSA

PEG

IND

GRU

CEP

OCT

CYG

CYG

IND

CEP

CAP

GRU

GRU

22 02.4

22 02.1

22 02.1

22 02.0

22 02.0

22 01.0

22 00.7

22 00.7

22 00.5

21 58.8

21 56.2

21 55.4

21 54.6

21 53.7

21 53.3

21 52.7

21 52.2

21 50.8

21 49.8

21 49.3

21 49.3

21 48.3

21 48.2

21 48.1

21 46.1

21 45.9

21 44.3

21 44.0

21 43.9

21 41.3

21 41.3

21 40.4

21 40.3

21 40.2

18 56

51 45

31 59

31 58

31 52

13 16

43 25

þ17 44

24 38

þ54 49

49 32

34 49

þ02 57

þ62 36

47 53

48 15

55 34

70 20

34 53

60 43

60 37

34 57

þ22 10

50 34

48 21

þ65 48

75 07

þ53 43

þ54 37

63 54

þ66 06

23 11

42 32

42 32

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC

GX

OC

OC

GX

OCþDN

GC

GX

GX

12.0

11.9

11.5

11.9

11.8

12.2

11.8

11.2

12.2

–

12.2

12.3

12.5

6.1

11.1

10.9

11.7

11.7

11.7

11.8

12.2

12.1

12.4

12.4

12.5

9.3

11.3

9.7

–

11.9

11.5p

6.9

11.6

11.4 0

0

0

0

0

0

0

3.80  1.10

1.9  1.4

0

0.80

1.2  0.9

0

2.40  1.30

2.6  1.5

0

2.40  0.90

3.2  2.1

0

h 2142

h 2138

12, 19, 20, 25

26

20, 25

20, 25

20, 25

12, 19, 20

20, 25, 26

6, 11, 12, 19

20, 25 0

2, 5

26

20, 25, 26

19

2, 5

– h 2139

h 2135

20, 25, 26

25, 26

26, 29

26, 29, 30

20, 25, 26

1.70  1.30

2.30  2.00

2.2  1.8

0

1.70  1.40

5.0

0

2.50  2.30

3.7  3.6

0

4.10  3.00

3.0  1.1

0

2.10  1.80

3.0  2.1

26, 29

26, 29

0

2.80  1.30 0

20, 25, 26

1.60  1.50

h 2136

26 11

h 2132

1.60  1.40

2.8  1.1

0

0

25, 26

12.00 1.40  1.10

26, 30 2, 5

4.00  2.60 h 2134

2, 5

6.0

2, 5

26, 29

1, 2, 5

4.00 h 2130

Small Cluster Nebula, h 2131

25

20, 25, 26

20, 25, 26

0

1.80  1.60

7.0

0

12.00

1.8  1.2

0

4.00  3.30

180 7219 7225 7229 7245 7243 7232

h 3927

h 3929

h 3930

H VI-29

H VIII-75 *

h 3931

7314

7302

H IV-31

h 3949

GRU

7284

H II-469 7307

7296

H VII-41 *

7309

7280

H II-248

h 3947

7281

h 2161

H II-476

AQR

7267

h 3938

CEP

PSA

AQR

AQR

LAC

PEG

CEP

PSA

AQR

7261 7252

H III-458

LAC

GRU

GRU

LAC

LAC

PSA

PSA

TUC

IND

CEP

PSA

AQR

PSA

GRU

IND

PEG

IND

LAC

IND

IND

PEG

AQR

AQR

Con

h 2159

7233

7216

h 3925

7248

7235 ¼ 7234

h 2154 ¼ H VIII-63

H III-863

7221

h 3928

h 3932

7214

7213

h 3924 7218

7205

h 3919

H II-897

7217

H II-207 *

h 3926

7196

h 3915

7179

h 3907 7192

7193

h 2145

7209

7185

h 2144

H VII-53 *

7184

H II-1

h 3914

NGC/M

Herschel

22 35.8

22 34.3

22 33.8

22 32.4

22 28.6

22 28.2

22 26.5

22 24.7

22 24.3

22 20.7

22 20.4

22 16.9

22 15.8

22 15.7

22 15.3

22 15.3

22 14.0

22 13.2

22 13.1

22 12.6

22 12.6

22 11.3

22 10.2

22 09.1

22 09.3

22 08.5

22 07.9

22 06.0

22 05.2

22 06.8

22 04.8

22 03.6

22 03.1

22 02.7

26 03

10 21

40 57

14 07

24 51

þ52 17

þ16 09

þ57 50

33 41

24 41

þ58 05

þ40 30

45 51

45 51

þ49 53

þ54 20

29 25

26 09

64 51

68 40

þ57 17

30 37

16 40

27 49

47 10

57 25

þ31 22

50 07

þ46 30

64 19

64 03

þ10 49

20 28

20 49

RA (2000.0) Dec

GX

GX

GX

GX

GX

OC

GX

OC

GX

GX

OC

GX

GX

GX

OC

OC

GX

GX

GX

GX

OC

GX

GX

GX

GX

GX

GX

GX

OC

GX

GX

OC/NE

GX

GX

Type

10.8

12.5

12.2

12.3

12.0

9.7p

12.1

–

12.0

11.1

8.4

12.5

12.2

12.0

6.4

9.2

12.5

12.3

12.4

12.5

7.7

12.1

12.0

12.5

10.1

10.8

10.2

11.4

7.7

11.2

12.5

–

12.2

11.1

Mag

20, 25

0

h 2165

4.60  2.00

20

20, 25, 26 12, 19, 20

3.4  1.0

2.00  1.70

12, 19, 20

20

2

6, 12, 19

0

0

h 2167

h 3943 1.80  1.10

2.3  1.6

0

0

4.00

2.1  1.5

0

2, 5 0

20, 25 h 2160

2, 5 20 12.00

h 3934

2, 6, 11

20, 25, 26

20, 25, 26

1.60  1.40

2.10  1.70

6.0

0

1.80  0.90

1.7  1.3

0

2

h 2155

30.00 2.60  1.00

20, 25 2

h 2157

5.00

20, 25

0

26, 29

26, 29, 30

1.80  1.50

2.0  1.0

0

1.70  1.00

1.7  1.0

0

2, 5

0

20, 25

4.00

12, 19, 20

2.00  1.60

2.60  1.10

2.2  1.4

h 2150

20, 25, 26

0

3.10  2.80 0

26, 29

4.00  2.00

26 6, 11

h 2149

2, 6, 11

6, 12, 19

26, 29

4.00  3.40

0

26, 29

20, 25

20, 25

Map no.

2.50  1.90

15.00

1.9  1.8

0

2.00  0.80

5.0

0

h 2147

h 2143

5.90  1.30 2.30  1.50

Name/Notes

Size

181

7448 7457 7454 7465

h 3962

H II-251 *

H II-212

H II-249

H III-211

7469

7417

h 2196

H III-230

7438

h 3965

7462

7424

h 3964

h 3968

7421

h 3963

7456

7418

H III-576

h 3966 ¼ h 3967

7429 7426

h 2139

7410 7412

h 3960

7419

H VII-43

h 3961

7392

H II-702

LAC

7394

7386

H III-217 7391

7385

H III-216

h 2188

7377

H II-598

H II-443

PEG

7380

H VIII-77 *

GRU

PEG

GRU

GRU

PEG

PEG

PEG

PEG

TUC

CAS

GRU

GRU

GRU

LAC

CEP

GRU

GRU

CEP

AQR

AQR

PEG

AQR

CEP

AQR

7368 7371

H II-477

PSA

TUC

CEP

CEP

PEG

PEG

PEG

h 3955

7329 7361

h 3851

h 3954

7352 7354

7339

H II-234

H II-705

7332

H II-233

h 2177

7331

H I-53 *

23 03.3

23 02.8

23 02.1

23 02.0

23 01.1

23 01.0

23 00.1

22 57.8

22 57.6

22 57.3

22 56.9

22 56.6

22 56.1

22 55.9

22 55.8

22 55.0

22 54.3

22 51.8

22 50.7

22 50.6

22 50.0

22 49.9

22 47.8

22 47.0

22 46.1

22 45.6

22 42.3

22 40.5

22 40.4

22 39.7

22 37.8

22 37.4

22 37.1

þ08 52

40 50

39 35

þ15 58

þ16 23

þ30 09

þ15 59

65 02

þ54 21

41 04

37 21

37 02

þ36 21

þ59 59

42 39

39 40

þ60 50

20 36

01 31

þ52 10

þ11 42

þ11 36

22 19

þ58 06

11 00

39 20

30 03

66 28

þ61 17

þ57 24

þ23 47

þ23 48

þ34 25

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

GX

GX

OC

GX

GX

OC

GX

GX

OC/NE

GX

GX

GX

OCþDN

GX

GX

GX

GX

PN

OC/NE

GX

GX

GX

12.0

11.4

11.7

12.3

11.8

11.0

11.4

12.4

10.2

11.7

11.0

12.4

–

11.1

10.4

13.0

11.8

12.2

–

12.5

12.2

11.0

7.2

11.6

12.4

12.3

11.6

12.2

–

12.3

11.0

9.5 0

3.7  2.7

h 2184

15.0

2, 5

20, 25

4.30  2.30 2.20  1.80

1.4  1.0

12

20, 26 0

4.30  0.80 0

20, 26

5.50  1.60 h 2204

6, 12 6, 12

2.20  1.60 h 2203

h 2201

2.60  1.20

6

26 6, 12, 19

h 2199

2.40  1.60

2

–

9.5  8.1

0

20 0

20 2.00  1.90

6 3.50  2.60

1.70  1.40

h 2192

20, 26 0

5.2  1.6

20, 26

2, 5

20

3.80  2.80

h 2190

6.00

12, 19

2

6, 12, 19

6, 12, 19

20

2

12, 19, 20

20, 26

20

26, 29

0

h 2186

2.20  1.40 0

h 2185

1.70  1.50

8.0  5.0

0

0

h 2183

1.3  1.1 1.80  1.10

h 2181

3.00  2.50 0

CH 19, h 2182

20.00 0

h 2180

0

2.00

2.9  0.6

0

3.90  1.00

0

2, 5

0

2

6

6

6

– h 2178

h 2173

h 2172

0.60

2.80  0.70

4.1  1.1

0

10.20  4.20

182 AQR GRU

7541 7531 7550 7562 7552 7585

h 3975

H III-181

H II-467

h 3977

H II-236

PEG TUC

7637 7680 7678 7676 7686

h 3984

H III-860

H II-226

h 3995

H VIII-69 *

TUC

AND

PEG

OCT

AND

7650 7662

H IV-18 *

CAS

GRU

AND

PEG

CAS

PEG

PEG

GRU

h 3989

7632

7640

H II-600 7654/M 52

7626

H II-440

h 3985

7635

H IV-52

h 2238

7625

H II-250

GRU

7599 7619

h 3981

7606

H I-104 *

H II-439

AQR

7590

h 3980

AQR

7582 7600

h 3978

H II-431

GRU

PSC

PEG

GRU

PSC

CEP

PEG

SCL

CEP

H II-430

7507

H II-2 7515

7510

H VII-44 *

GRU

7538

7496

h 3973

PEG

H III-220

7497

H III-203 *

AQR

SCL

PEG

Con

H II-706

7484 7492

h 3971 ¼ h 3972

7479

H I-55 *

H III-558

NGC/M

Herschel

23 30.2

23 28.9

23 28.5

23 28.5

23 26.5

23 25.9

23 25.3

23 24.2

23 22.1

23 22.1

23 20.7

23 20.7

23 20.5

23 20.2

23 19.3

23 19.1

23 18.9

23 18.9

23 18.4

23 18.0

23 16.2

23 16.0

23 15.3

23 14.8

23 14.7

23 13.5

23 12.9

23 12.1

23 11.5

23 09.8

23 09.1

23 08.4

23 07.1

23 04.9

þ49 08

59 43

þ22 25

þ32 24

81 55

þ42 33

57 48

þ61 35

42 30

þ40 51

þ08 13

þ61 12

þ17 14

þ08 12

42 15

08 29

42 14

07 35

42 22

04 39

42 35

þ06 41

þ18 57

43 36

þ04 32

þ61 31

þ12 41

28 32

þ60 34

43 26

þ18 11

15 37

36 16

þ12 19

RA (2000.0) Dec

OC

GX

GX

GX

GX

PN

GX

OC

GX

GX

GX

DN

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

DN

GX

GX

OC

GX

GX

GC

GX

GX

Type

5.6

11.7

11.8

12.5

12.5

8.3

12.5

6.9

12.1

11.1

11.2

11.0p

11.9

11.1

11.5

10.8

11.3

11.9

10.5

11.4

10.6

11.6

12.2

11.3

11.7

–

12.5

10.4

7.9

11.1

12.3

11.2

11.2

10.9

Mag h 2205

0

0

h 2219 h 2223

0

15.00

1.6  0.9

0

0

2.50  1.70

1.9

0

2.10  1.90

0.60

1.4  1.1

0

16.00

2.4  1.2

0

h 2249

h 2245

h 2246

Blue Snowball, h 2241

h 2236

10.50  1.80 0

h 2233

2.60  2.30

h 2232 Bubble Nebula, h 2235

0

h 2230 15.00  8.00

1.6  1.4

0

2.50  2.30

4.4  1.4

0

in GRU Quartet

h 2228 ¼ h 3982 0

in GRU Quartet

2.6  1.0

5.40  2.10

h 2227 0

0

2.50  1.00

5.0  2.3

0

in GRU Quartet

h 2226 ¼ h 3979 0

in GRU Quartet

2.30  2.00

3.4  2.7

0

0

1.4  1.2 2.20  1.70

h 2216

h 2214

h 2211 ¼ h 3974

0

0

4.50  1.70

3.5  1.2

0

9.00  6.00

1.7  1.6

0

2.80  2.70

7.0

0

h 2213

h 2209

4.40  1.70 3.30  3.10

h 2208

1.8  1.7 4.20

0

4.00  3.10 0

Name/Notes

Size

2, 6

26

6

6

30

2, 6

26

2

20, 26

2, 6

12

2

6, 12

12

20, 26

12

20, 26

12

20, 26

12

20, 26

12

6, 12

20, 26

12

2

6, 12

20

2, 5

20, 26

6, 12

12, 20

20

6, 12

Map no.

183 7795 7796 7798

h 2287

h 4009

H II-232

7789

H VI-30 * 7790

7788

h 2283

H VII-56 *

7785

H II-468

PEG

7772 7782

h 2276

7771

H III-233

PEG

7769

PEG

PHE

CAS

CAS

CAS

CAS

PSC

PSC

PEG

PHE

PEG

CEP

PSC

SCL

PEG

H II-231

7755

h 4005

H II-230

7753

H II-213

PHE

CEP

7764

7744

h 4003

h 4006

7748

h 2266

PEG

PEG

7768

7743

H II-256

h 2273

7742

H II-255

PEG

AQR

7757

7741

H II-208

7762

7727

H I-111 *

AQR

H VII-55

7723

H I-110 *

AQR

PEG

SCL

PSC

PSC

PEG

PHE

CEP

PHE

PHE

h 2270

7721

h 2258

H II-432

7716

h 2257 7713

7714

H II-244

7720

7711

h 3999

H III-146

7702

H VIII-62

h 4000

7690 7708

h 3997

7689

h 3996

23 59.4

23 59.0

23 58.7

23 58.4

23 57.0

23 56.7

23 55.3

23 53.9

23 51.8

23 51.4

23 51.1

23 50.9

23 50.9

23 49.8

23 48.8

23 47.9

23 47.1

23 45.0

23 45.0

23 44.4

23 44.3

23 43.9

23 39.9

23 38.9

23 38.8

23 38.5

23 36.5

23 36.5

23 36.2

23 35.7

23 35.4

23 34.3

23 32.9

23 32.7

þ20 45

55 27

þ60 00

þ61 13

þ56 44

þ61 24

þ05 55

þ07 58

þ16 15

þ20 07

þ20 09

40 44

þ27 10

þ68 02

þ04 10

30 31

þ29 29

42 55

þ69 45

þ09 56

þ10 46

þ26 05

12 18

12 58

06 31

þ27 02

37 56

þ00 18

þ02 09

þ15 18

56 00

þ72 55

51 41

54 05

GX

GX

OC/NE

OC

OC

OC

GX

GX

OC

GX

GX

GX

GX

OC

GX

GX

GX

GX

DN/NE

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

GX

OC/NE

GX

GX

12.3

11.5

–

8.5

6.7

9.4

11.6

12.3

–

12.1

12.0

12.3

12.3

10.0

12.4

11.7

12.2

11.9

7.1p

11.4

11.6

11.0

10.6

11.2

11.6

12.4

10.9

12.0

12.2

12.1

12.2

–

12.2

11.5 26

12

h 2274 h 2275

2.40  1.10

h 2285

5.00

2 26 6

– 2.20  1.90 1.40  1.30

h 229

2 2

2 Caroline’s Cluster, CH 14, h 2284

12 25.00

h 2282

2.50  1.30

12

6, 12

6, 12

6, 12

4.00

h 2281

2.20  1.30

5.0

0

3.2  2.7

0

0

20

2 6

h 2272

20

2.00  1.50

0

6

1.60  1.30

15.00

2.4  1.7

0

3.80  2.80

3.3  2.1

0

20, 26

0

2 h 2268

6, 12 12

2.20  1.80

h 2264

6

12, 20

12, 20

12

6

–

2.80  2.40

1.7

0

4.50  2.90

4.7  3.5 h 2262

h 2261

3.50  2.20 0

h 2260

2.80  1.10 0

h 2259

1.60  1.30

4.5  1.8

20

12

0

2.20  1.80 0

12

1.90  1.40

26

1, 2 6, 12

h 2256

h 2255

26

2.60  1.30

0

2.10  1.20

–

2.1  0.8

0

2.80  1.90