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Spatial Distribution of Globular Clusters in M 31

Published online by Cambridge University Press:  19 July 2016

Jun-Ichi Watanabe  and
Tomohiko Yamagata
Jun-Ichi Watanabe
Affiliation:
Tokyo Astronomical Observatory
Tomohiko Yamagata
Affiliation:
Tokyo Astronomical Observatory

Abstract

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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.

Type
Chapter VIII. Poster Papers on Cluster Systems in Nearby Galaxies
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 551 - 552
Copyright
Copyright © Kluwer 1988 

References

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