Imprint of galaxy formation and evolution on globular cluster properties

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dc.creatorBekki, Kenji
dc.date2006-05-13
dc.date.accessioned2026-07-07T07:08:26Z
dc.date.available2026-07-07T07:08:26Z
dc.descriptionWe discuss the origin of physical properties of globular cluster systems (GCSs) in galaxies in terms of galaxy formation and evolution processes. Based on numerical simulations of dynamical evolution of GCSs in galaxies, we particularly discuss (1) the origin of radial density profiles of GCSs, (2) kinematics of GCSs in elliptical galaxies, (3) transformation from nucleated dwarf galaxies into GCs (e.g., omega Centauri), and (4) the origin of GCSs in the Large Magellanic Cloud (LMC).
dc.description8 pages, 4 figures, Conference proceedings for an invited talk at ESO conference ``Globular clusters - Guides to galaxies''
dc.identifierhttps://arxiv.org/abs/astro-ph/0605335
dc.identifierhttp://arxiv.org/abs/astro-ph/0605335
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110704
dc.subjectAstrophysics
dc.titleImprint of galaxy formation and evolution on globular cluster properties
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