A Unified N-Body and Statistical Treatment of Stellar Dynamics - Part Two - Applications to Globular Cluster Cores

Details A Unified N-Body and Statistical Treatment of Stellar Dynamics - Part Two - Applications to Globular Cluster Cores A Unified N-Body and Statistical Treatment of Stellar Dynamics - Part Two - Applications to Globular Cluster Cores

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283..813m&link_type=abstract

Astrophysical Journal, Vol.283, NO.2, P. 813, 1984

Astronomy and Astrophysics

Astrophysics

26

Scientific paper

The auhors apply their new "hybrid" stellar dynamical computer code to the gravitational collapse and post collapse evolution of a globular cluster, in the approximation of point particles of initially equal mass and for a time equal to twice the time to collapse. Among the results is the formation of a hard central binary system, reversal of core collapse and expansion due to the heat input from this binary, ejection of the binary from the core, and recollapse of the core.

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