An Atlas of Local Group Galaxies by Paul W. Hodge

By Paul W. Hodge

This atlas offers an entire set of pictures of neighborhood crew Galaxies and exhibits an important gadgets, together with many person stars and interstellar gadgets. items pointed out in a few two hundred charts contain variable stars, globular superstar clusters, open celebrity clusters, dirt clouds, and supernova remnants. every one galaxy is followed by means of 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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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.

M33 Star Clusters Cluster a Other Name Chart ------ 13 16 16 18 18 6 7 8 9b 10 ---CS 37 -- 15 15 12 15 12 11 12 13 14 15 15 12 15 12 12 16 17 18 19 20 CS 38 -CS 36 -------CS 24 12 9 5 12 9 21 22 23 24 25 CS 1 CS 23 ---- 5 9 15 9 12 26 27 28 29 30 ---- 12 9 5 11 0 MO 1 2 3 4 5 CS 35 -- 18 31 32 33 34 35 CS 17 ----- 9 14 8 8 11 36 37 38 39 40 41 42 43 44 45 CS 33 ---------- 11 8 11 8 8 11 11 14 8 8 46 47 48 49 50 ---CS 18 CS 16 11 11 11 8 8 51 52 54 55 56 CS 39 CS 13 CS 27 CS 20 -- 14 8 8 8 8 58 CS 2 3 4 6 ------ 3 4 4 4 5 7 8 9 10 11 ------ 6 5 9 9 9 12 -- 8 19 a 14 15 19 21 ----- 4 8 8 9 22 25 26 28 29 ------ 7 9 9 9 8 30 31 32 34 ----- 8 9 11 13 MO = Melnick and D’Odorico (1978); CS = Christian and Schommer (1982).

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). , 1997). c SNR candidates are from Sabbadin (1979, identified with prefix S), D’Odorico, Dopita, and Benvenuti (1980, prefix DDB), and Gordon et al.

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