By Paul W. Hodge
This atlas presents a whole set of pictures of neighborhood workforce Galaxies and indicates crucial items, together with many person stars and interstellar gadgets. gadgets pointed out in a few two hundred charts contain variable stars, globular megastar clusters, open superstar clusters, dirt clouds, and supernova remnants. each one galaxy is observed through an in depth bibliography. The atlas comes in handy for researchers, scholars, and beginner astronomers. The authors are affiliated with the college of Washington. there isn't any topic index.
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Additional info for An Atlas of Local Group Galaxies
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.
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.
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.