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Shapes of Magellanic Cloud star clusters
Published online by Cambridge University Press: 19 July 2016
Abstract
The ellipticities of the most populous MC star clusters (87) have been derived for studying a) ellipticity variations within individual clusters, b) variations of ellipticity distributions for various galaxies, and c) variations of ellipticity of star clusters relative to their dynamical parameters.
From the studied clusters it is found that radial ellipticity variations within individual clusters seem to be a common phenomenon for the MC clusters where the inner parts are more elliptical than the outer. The SMC clusters are more elliptical than LMC clusters where ellipticities are measured at rh.
The dynamical masses of the clusters seem to correlate with ellipticities where the most massive are the most elliptical.
- Type
- Star Formation and Clustering
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 234 - 235
- Copyright
- Copyright © Kluwer 1991
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