Dynamical masses, time-scales, and evolution of star clusters

Simple item page
dc.creatorGerhard, Ortwin
dc.date2000-07-18
dc.date.accessioned2026-07-07T01:54:26Z
dc.date.available2026-07-07T01:54:26Z
dc.descriptionThis review discusses (i) dynamical methods for determining the masses of Galactic and extragalactic star clusters, (ii) dynamical processes and their time-scales for the evolution of clusters, including evaporation, mass segregation, core collapse, tidal shocks, dynamical friction and merging. These processes lead to significant evolution of globular cluster systems after their formation.
dc.descriptionInvited review, 13 pages, LaTeX. To appear in Massive Stellar Clusters, ed. A. Lancon, C.M. Boily, ASP, 211, 12, 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0007258
dc.identifierhttp://arxiv.org/abs/astro-ph/0007258
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1349
dc.subjectAstrophysics
dc.titleDynamical masses, time-scales, and evolution of star clusters
dc.typetext

Files

Collections

arXiv