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The Early Stages of Post-Collapse Cluster Evolution
Symposium - International astronomical union
We present here some recent (and very preliminary) findings from a study of the early stages of the post-core-collapse evolution of an isolated cluster of identical point "stars". The method used to follow the behavior of the system is the unified N-body/statistical treatment described in detail by McMillan and Lightman (1984a) and by Lightman and McMillan elsewhere in this volume. Briefly, the method combines the standard "large-N" and "small-N" approaches to the problem in the régimes wheredoi:10.1017/s0074180900147552 fatcat:3stbr7v74rdtnepdcgupgkebhi