NUMERICAL MODELING OF GLOBULAR CLUSTERS TIDAL DISSOLUTION

Numerical model of dynamical evolution of globular clusters(GCs) is described, with an emphasis of the mass loss rate in tidal interactions with the Galaxy. On a set of models dependence of the tidal destruction on cluster parameter sand initial conditions, such as: the initial cluster mass, its ini...

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Bibliographic Details
Main Authors: M. V. Ryabova, F. G. Sendzikas, Yu. A. Shchekinov
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2013-11-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/82273