The Impact of Rotation on Cluster Dynamics
| dc.creator | Boily, Christian | |
| dc.date | 2000-02-23 | |
| dc.date.accessioned | 2026-07-07T01:52:27Z | |
| dc.date.available | 2026-07-07T01:52:27Z | |
| dc.description | 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. | |
| dc.description | Talk given at the Strasbourg meeting Massive Star Clusters in November 1999; 7 pages, 3 figures xv-8bit giffed and tarred (= 100Kbytes); newpasp style file included | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0002428 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0002428 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/624 | |
| dc.subject | Astrophysics | |
| dc.title | The Impact of Rotation on Cluster Dynamics | |
| dc.type | text |