By Paul W. Hodge
This Atlas presents an entire set of pictures of neighborhood staff Galaxies (excluding the 3 for which id atlases are already in print) and exhibits an important items, together with many hundreds of thousands of person stars and interstellar objects.
It is exclusive in its assurance and layout and gives a resource of those basic information that may be used for a few years. Researchers, scholars or even beginner astronomers might be in a position to use the Atlas to spot and learn some of the parts of the approximately 30 vital galaxies lined via the Atlas.
The items pointed out at the greater than two hundred charts contain variable stars, globular famous person clusters, open famous person clusters, stellar institutions, emission areas, supernova remnants, planetary nebulae and dirt clouds. every one galaxy is followed through an in depth bibliography.
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Extra info for An Atlas of Local Group Galaxies
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. M33 Emission Regions Identified by Courtès et al.
53 Table 4b. M33 Emission Regions Identified by Courtès et al.
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. 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.