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The Impact of Rotation on Cluster Dynamics

Christian Boily
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Abstract

The evolution of rotating, isolated clusters of stars up to core-collapse is investigated with n-body numerical codes. The simulations start off from axisymmetric generalisations of King profiles, with added global angular momentum. In this contribution I report on results obtained for two sets of single-mass cluster simulations. These confirm the more rapid evolution of even mildly-rotating clusters. A model is presented with rotational energy comparable to omega-Centauri's; it reaches core-collapse in less than half the time required for non-rotating model clusters.

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Christian Boily. 2000-02-23. The Impact of Rotation on Cluster Dynamics. https://arxiv.org/abs/astro-ph/0002428

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