The Structure of Rapidly Rotating Relaxed Globular Clusters

Details The Structure of Rapidly Rotating Relaxed Globular Clusters The Structure of Rapidly Rotating Relaxed Globular Clusters

Jul 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..12...47k&link_type=abstract

Astrophysics and Space Science, Volume 12, Issue 1, pp.47-57

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

A model of rapidly rotating globular clusters is constructed assuming uniform angular velocity and a truncated Maxwellian distribution in the stellar velocities. Since the first-order theory developed by Woolley and Dickens becomes inaccurate for rapid rotation, a small-mass envelope is fitted to their models by the method of Monaghan and Roxburgh. A comparison is made of the critical values derived by the two methods.

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