Early Evolution of Globular Clusters

Details Early Evolution of Globular Clusters Early Evolution of Globular Clusters

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.0701h&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #07.01; Bulletin of the American Astronomical Society, Vol. 34, p.1101

Astronomy and Astrophysics

Astronomy

Scientific paper

Using numerical simulations and a variety of initial conditions, we studied the evolution of young globular clusters. Our tree-based N-body code contains a novel implementation of algorithmic regularization to treat close encounters between stars. The results show that young globular clusters retain memory of their initial conditions, predominantly in the form of coherent orbital motion of stars in their halos. We investigate the possibility of determining these initial conditions with observations of young globular clusters in the Large Magellanic Cloud.

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