An Atlas of Local Group Galaxies by Paul W. Hodge

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. items pointed out in a few two hundred charts comprise variable stars, globular superstar clusters, open celebrity clusters, airborne dirt and dust clouds, and supernova remnants. each one galaxy is followed through an in depth bibliography. The atlas turns out to be useful for researchers, scholars, and novice astronomers. The authors are affiliated with the collage of Washington. there is not any topic index.

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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. items pointed out in a few two hundred charts comprise variable stars, globular superstar clusters, open celebrity clusters, airborne dirt and dust clouds, and supernova remnants. each one galaxy is followed through an in depth bibliography. The atlas turns out to be useful for researchers, scholars, and novice astronomers. The authors are affiliated with the collage of Washington. there is not any topic index.

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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.

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.

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.

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