Fitting Dynamical Models to Observations of Globular Clusters

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dc.creatorMcLaughlin, Dean E.
dc.date2003-02-14
dc.date.accessioned2026-07-07T02:07:36Z
dc.date.available2026-07-07T02:07:36Z
dc.descriptionThe basic ingredients of models for the internal dynamics of globular clusters are reviewed, with an emphasis on the description of equilibrium configurations. The development of progressive complexity in the models is traced, concentrating on the inclusion of velocity anisotropy, rotation, and integrals of motion other than energy. Applications to observations of extragalactic globulars and to combined radial-velocity and proper-motion datasets are discussed.
dc.description16 pages, to appear in New Horizons in Globular Cluster Astronomy, ed. G. Piotto et al
dc.identifierhttps://arxiv.org/abs/astro-ph/0302283
dc.identifierhttp://arxiv.org/abs/astro-ph/0302283
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5747
dc.subjectAstrophysics
dc.titleFitting Dynamical Models to Observations of Globular Clusters
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