Early evolution of Globular Clusters

Details Early evolution of Globular Clusters Early evolution of Globular Clusters

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..4cf.1a014h&link_type=abstract

American Physical Society, Four Corners Meeting 2002, October 4-5, 2002 University of Utah, Salt Lake City, Utah, MEETING ID: 4C

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Scientific paper

Most of the previous numerical studies were concentrated on the calculation of late evolution because of oldness of Globular Clusters(GCs) in the Milky Way galaxy. On the other hand, GCs in the large megellanic cloud(LMC) are much younger than ones in Milky Way. Since stars in GCs are considered to be born simultaneously, the early stage of GCs' evolution in LMC may keep the information of star formation region. We show the initial condition dependence of the early evolution of GCs using N-body simulation with regularization for particles in close encounter.

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