Internal rotation of young globular clusters

Details Internal rotation of young globular clusters Internal rotation of young globular clusters

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..14e..37v&link_type=abstract

Modelling Dense Stellar Systems, 26th meeting of the IAU, Joint Discussion 14, 22-23 August 2006, Prague, Czech Republic, JD14,

Physics

Scientific paper

We report the results of N-body simulations of the early evolution of globular clusters and show how the kinematical properties of clusters emerging at the end of the violent relaxation are affected by the motion of a cluster in its host galaxy and by the host galaxy tidal field. In particular, we discuss the properties and the origin of the internal rotation velocity produced during this stage.

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