Masses and Relaxation Times of Star Clusters in the Small Magellanic Cloud

Details Masses and Relaxation Times of Star Clusters in the Small Magellanic Cloud Masses and Relaxation Times of Star Clusters in the Small Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108...25k&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

1

Scientific paper

Plates taken with the 1.2-m U.K. Schmidt Telescope and the 3.8-m AAT have been used in order to derive the dynamical parameters of 43 various clusters of the SMC by means of star counts. The clusters are divided into two categories: (1) the disk clusters and (2) the halo globular clusters. The disk clusters are found to be more massive and older than the galactic open clusters, whereas the halo clusters are at least 10 times less massive than the galactic globulars.

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