The Imprints of IMBHs on the Structure of Globular Clusters: Monte-Carlo Simulations

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dc.creatorUmbreit, Stefan
dc.creatorFregeau, John M.
dc.creatorRasio, Frederic A.
dc.date2008-03-06
dc.date.accessioned2026-07-07T09:25:09Z
dc.date.available2026-07-07T09:25:09Z
dc.descriptionWe present the first results of a series of Monte-Carlo simulations investigating the imprint of a central black hole on the core structure of a globular cluster. We investigate the three-dimensional and the projected density profile of the inner regions of idealized as well as more realistic globular cluster models, taking into account a stellar mass spectrum, stellar evolution and allowing for a larger, more realistic, number of stars than was previously possible with direct N-body methods. We compare our results to other N-body simulations published previously in the literature.
dc.descriptionto appear in the proceedings of IAUS 246, "Dynamical Evolution of Dense Stellar Systems", eds. Vesperini, Giersz and Sills. 5 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/0803.0781
dc.identifierhttp://arxiv.org/abs/0803.0781
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/156311
dc.subjectAstrophysics
dc.titleThe Imprints of IMBHs on the Structure of Globular Clusters: Monte-Carlo Simulations
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