Spatial Distribution of Globular Clusters in M 31
1988 ◽
Vol 126
◽
pp. 551-552
The spatial distribution of globular clusters in M 31 has been analyzed using the catalogues of Sargent et al. (1977) and Crampton et al. (1985). It is concluded that the globular clusters within the distance of 54′ from the center of M 31 show an elliptical distribution aligned to the major axis of the disk. This is similar to the distribution of metal-rich clusters in our galaxy.
2006 ◽
Vol 449
(1)
◽
pp. 143-149
◽
Keyword(s):
1996 ◽
Vol 169
◽
pp. 669-680
1993 ◽
Vol 153
◽
pp. 323-324
Keyword(s):
2011 ◽
Vol 531
◽
pp. A155
◽
2009 ◽
Vol 500
(2)
◽
pp. 769-779
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2004 ◽
Vol 194
◽
pp. 240-240
Keyword(s):