The role of three-body stability in tidally interacting globular clusters

被引：0
|
作者：
Kennedy, Gareth F. [1 ,2 ]
机构：
[1] Chinese Acad Sci, Natl Astron Observ China, Beijing 100012, Peoples R China
[2] Monash Univ, Monash Ctr Astrophys, Clayton, Vic 3800, Australia
来源：
STAR CLUSTERS AND BLACK HOLES IN GALAXIES ACROSS COSMIC TIME | 2016年 / 10卷 / 312期
关键词：
gravitation; stellar dynamics; methods: analytical; stars: kinematics; globular clusters: general; I;
D O I：
10.1017/S1743921315007863
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The role of stability in the general three-body problem is investigated with regard to the tidal radius of a globular cluster (GC) in a galactic potential. This proceedings is a summary of two papers which outline the stability method (Kennedy 2014a) and compare the predicted stability boundary radius to observations of velocity dispersion profiles in Milky Way GCs (Kennedy 2014b).
引用
收藏
页码：231 / 234
页数：4
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