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By Paul W. Hodge

This atlas offers an entire set of pictures of neighborhood team Galaxies and exhibits crucial gadgets, together with many person stars and interstellar items. items pointed out in a few two hundred charts comprise variable stars, globular famous person clusters, open celebrity clusters, dirt clouds, and supernova remnants. each one galaxy is observed via an in depth bibliography. The atlas turns out to be useful for researchers, scholars, and beginner astronomers. The authors are affiliated with the collage of Washington. there isn't any topic index.

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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.

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).

28325 -30 28 24501 24533 24599 24798 24838 ----SC G14 28 31 28 30 28 24858 24887 25017 25060 25061 H 33 --VHK 80 -- 28 30 28 31 31 25201 25255 25615 25620 25933 ------ 28 28, 31 26 28 31 25987 26066 26163 26166 26175 ---H 35,VHK 35, SC E7 -- 28 30 31 28 28 26195 26212 26348 26414 26428 --H 32 --- 31 28 28 31 31 26477 26524 26647 26729 26788 -SC B1 ---- 30 26 31 28 30 26850 26910 --- 31 26 30 27065 27330 27544 ---- 31 31 28 27608 27639 27689 27697 27777 ------ 31 30 31 28 29 27830 27840 28021 28065 28168 -SC E34 SC E17 -VHK 58 28 26 26 28 28 28325 28367 28500 28578 28632 24472 ----- 28 31 26 31 31 28639 28664 28706 28768 28785 ----- SC F12 28 28 31 28 29 28834 28986 28988 29032 29104 SC G14 VHK 55 ---- 28 26 31 26 31 29131 29211 29250 29280 29334 ------ 31 31 31 29 31 29397 29476 --- 28 28 31 29618 29631 29799 ---- 28 31 28 29926 30001 30125 30133 30173 ------ 28 31 28 28 28 30352 30422 30459 30526 30718 ---VHK 69 -- 31 31 31 31 31 30804 31100 31267 31396 31458 ------ 29 31 31 28 31 31668 31786 31805 31929 31953 VHK 57 ---SC G6 31 28 28 26 31 31986 32023 32117 32202 32473 ----SC F9 28 31 28 28 29 33070 33350 34052 34497 35284 SC F8 ----- 29 26 31 31 31 35369 36117 --- 31 26 32 a 36568 36781 36806 ---- 31 32 32 36841 37040 --- 26 26 The variable stars are all based on the Kinman, Mould and Wood (1987) survey and are identified by the numbers in that catalog (designation: KMW), which also provided the alternate names given here (designation VHK: van den Bergh, Herbst, Kowal (1975); H: Hubble (1926); HS: Hubble and Sandage (1953); SC: Sandage and Carlson (1983)).

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