Dynamical Simulations: Methods and Comparisons

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dc.creatorHeggie, D. C.
dc.creatorGiersz, M.
dc.creatorSpurzem, R.
dc.creatorTakahashi, K.
dc.date1997-11-17
dc.date.accessioned2026-07-07T02:25:08Z
dc.date.available2026-07-07T02:25:08Z
dc.descriptionWe review recent progress in computational methods for studying the dynamical evolution of large star clusters. After describing some highlights of a new comparison of different models, including N-body models, we mention in detail recent developments in three codes which allow models with anisotropic distributions of velocity to be studied: (i) a Fokker-Planck code using finite differences, (ii) a Monte Carlo code and (iii) a gaseous model code.
dc.description6 pages, postscript, etc., also available at http://www.maths.ed.ac.uk/people/douglas/preprints.html To appear in Andersen J., ed, Highlights of Astronomy Vol. 11. Kluwer, Dordrecht. Pagination differs from that in published version
dc.identifierhttps://arxiv.org/abs/astro-ph/9711191
dc.identifierhttp://arxiv.org/abs/astro-ph/9711191
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11817
dc.subjectAstrophysics
dc.titleDynamical Simulations: Methods and Comparisons
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