Dynamical masses, time-scales and evolution of star clusters

被引：0
|
作者：
Gerhard, O [1 ]
机构：
[1] Univ Basel, Inst Astron, CH-4102 Binningen, Switzerland
来源：
MASSIVE STELLAR CLUSTERS | 2000年 / 211卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This 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.
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页码：12 / 24
页数：13
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