Abstract
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.
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© 1985 International Astronomical Union
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Stodółkiewicz, J.S. (1985). Monte-Carlo Calculations. In: Goodman, J., Hut, P. (eds) Dynamics of Star Clusters. International Astronomical Union. Symposium, vol 113. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5335-2_44
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DOI: https://doi.org/10.1007/978-94-009-5335-2_44
Publisher Name: Springer, Dordrecht
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