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 indicates an important items, together with many hundreds of thousands of person stars and interstellar objects.
It is exclusive in its insurance and layout and offers a resource of those basic facts that may be used for a few years. Researchers, scholars or even novice astronomers should be in a position to use the Atlas to spot and learn many of the parts of the approximately 30 very important galaxies lined by means of the Atlas.
The items pointed out at the greater than two hundred charts comprise variable stars, globular superstar clusters, open megastar clusters, stellar institutions, emission areas, supernova remnants, planetary nebulae and mud clouds. every one galaxy is followed by way of an in depth bibliography.
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Additional resources for An Atlas of Local Group Galaxies
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. M33 Emission Regions Identified by Courtès 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.
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.