By Paul W. Hodge

This Atlas presents a whole set of pictures of neighborhood workforce Galaxies (excluding the 3 for which identity atlases are already in print) and indicates an important gadgets, together with many hundreds of thousands of person stars and interstellar objects.

It is exclusive in its assurance and layout and offers a resource of those basic information that may be used for a few years. Researchers, scholars or even beginner astronomers should be in a position to use the Atlas to spot and research a number of the parts of the approximately 30 vital galaxies lined through the Atlas.

The gadgets pointed out at the greater than two hundred charts comprise variable stars, globular big name clusters, open famous person clusters, stellar institutions, emission areas, supernova remnants, planetary nebulae and dirt clouds. each one galaxy is observed through an in depth bibliography.

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C SNR candidates are from Sabbadin (1979, identified with prefix S), D’Odorico, Dopita, and Benvenuti (1980, prefix DDB), and Gordon et al. (1998, prefix G). Gordon et al. (1998) cross-reference various identifications of the SNRs. d BCLMP 660 appears as a complete ring in Figure 7b of Courtès et al. (1987). We detect only a partial ring in our images. e SNR DDB 18 is contained within BCLMP 750. Gordon et al. (1998) do not identify it with G97, but we believe they are the same object. 53 Table 4b.

We note that the fainter variables were often very difficult to identify with certainty and users should be aware of possible misidentifications. 33 Table 4a. M33 Emission Regions Identified by Boulesteix et al. 4 30 30 30 30 30 38 32 32 32 31 43 30 32 12 45 150 71 40 76 99 535 174 109 213 354 751 752 753 756 BCLMP emission regions are labeled on the M33 charts with their number and no prefix. Separate subcomponents of complex regions are given lowercase Arabic letters and are identified on Charts 59-83.

4 30 30 30 30 30 38 32 32 32 31 43 30 32 12 45 150 71 40 76 99 535 174 109 213 354 751 752 753 756 BCLMP emission regions are labeled on the M33 charts with their number and no prefix. Separate subcomponents of complex regions are given lowercase Arabic letters and are identified on Charts 59-83. , 1997). , 1997). c SNR candidates are from Sabbadin (1979, identified with prefix S), D’Odorico, Dopita, and Benvenuti (1980, prefix DDB), and Gordon et al. (1998, prefix G). Gordon et al. (1998) cross-reference various identifications of the SNRs.

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