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The Caldwell Objects

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(www.stsci.edu).<br />

D i f N f e u b s u e l a e<br />

<strong>The</strong> Deep Sky Field Guide to Uranometria<br />

2000.0.<br />

Sky Catalogue 2000.0, Vol. 2.<br />

G a l a x i e s<br />

Tully, R. Brent. Nearby Galaxies Catalog.<br />

Cambridge, England: Cambridge University<br />

Press, 1988. (types, angular sizes, distances,<br />

masses, and luminosities)<br />

<strong>The</strong> Deep Sky Field Guide to Uranometria<br />

2000.0. (apparent magnitudes and surface<br />

brightnesses)<br />

NASA Extragalactic Database. Pasadena, CA:<br />

Infrared Processing and Analysis Center.<br />

http://nedwww.ipac.caltech.edu/. (positions<br />

and, when not available from the above<br />

references, other parameters)<br />

E x t r a S g u a p l e a r c n t i o c v a e<br />

"List of Supernovae." Cambridge, MA: Central<br />

Bureau for Astronomical Telegrams.<br />

http://cfa-www.harvard.edu/iau/lists/<br />

Supernovae.html.<br />

Note that World Wide Web Uniform Resource<br />

Locators, or URLs, are subject to change.<br />

<strong>The</strong> dimensions, magnitudes, and positions of<br />

non-<strong>Caldwell</strong> objects generally were taken from<br />

<strong>The</strong> Deep Sky Field Guide to Uranometria 2000.0.<br />

Incidentally, the two-volume Uranometria 2000.0<br />

atlas was radically revised as this book went to<br />

press, as was its Deep Sky Field Guide companion;<br />

descriptions of Uranometria 2000.0 charts refer to<br />

previous incarnations.<br />

Finally, in Chapter 2 and Appendix A the<br />

<strong>Caldwell</strong> objects' celestial coordinates are stated<br />

to varying degrees of precision. In each case the<br />

decision was based on the object's angular<br />

12<br />

size and degree of concentration or symmetry<br />

(tiny planetary nebulae merit arcsecond precision,<br />

for example, while loose, 1°-wide open<br />

clusters are listed to the nearest arcminute). <strong>The</strong><br />

coordinates should get each <strong>Caldwell</strong> object into<br />

the field of view of a computer-driven telescope<br />

or an equatorially mounted one being aimed with<br />

the help of setting circles.<br />

Incidentally, you'll note that I do not refer to<br />

objects in this book as "C" objects, as in "C101." I<br />

spell out the name "<strong>Caldwell</strong>." For the same<br />

reason that Moore decided not to use the prefix<br />

"M" (because that would conflict with the<br />

Messier, or "M," objects), I decided not to call his<br />

picks "C" objects either. As Archinal points out,<br />

the "C" prefix has already been used for other<br />

astronomical catalogs and is widely recognized<br />

as a prefix designating star clusters. "<strong>The</strong><br />

Dictionary of Nomenclature of Celestial <strong>Objects</strong> .<br />

. . shows 13 catalogs already designated by the 'C<br />

name," he says. "In fact the Task Group on<br />

Astronomical Designations of IAU Commission 5<br />

specifically recommends... that among other<br />

things, 'an acronym shall consist of at least three<br />

characters.'" Thus for this book I have adopted<br />

Archinal's recommendation, and use the full<br />

<strong>Caldwell</strong> name. ("C" designations do appear on<br />

the detailed finder charts and some photos for<br />

brevity, however.)<br />

SOME ORIGINAL SINS<br />

This work corrects several unfortunate errors that<br />

appeared in the December 1995 issue of Sky &<br />

Telescope, where the <strong>Caldwell</strong> Catalog first was<br />

published. In several cases the tabular<br />

information (magnitudes, sizes, etc.) in this book<br />

also differs significantly from that found in the<br />

original Sky & Telescope presentation or on early<br />

editions of the popular <strong>Caldwell</strong> Card. Here are<br />

but a few of the most obvious errors that have<br />

been corrected in this book.<br />

Deep-Sky Companions: <strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong>

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