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Monte-Carlo Calculations

Published online by Cambridge University Press:  04 August 2017

J.S. Stodółkiewicz
J.S. Stodółkiewicz*
Affiliation:
N. Copernicus Astronomical Center, Warsaw, Poland

Abstract

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The evolution of a nonisolated globular cluster is presented. The binaries (both, tidally captured and formed in three-body interactions), outflow of mass from stellar envelopes and shocks are considered as sources of energy in the cluster.

Information

Type
May 31: External Fields and Finite-Star-Size Effects
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985, pp. 361 - 372
Copyright
Copyright © Reidel 1985 

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