Dynamical evolution of globular clusters in the magellanic clouds and other local systems

被引：0
|
作者：
Mackey, AD [1 ]
Gilmore, GF [1 ]
机构：
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
来源：
NEW HORIZONS IN GLOBULAR CLUSTER ASTRONOMY | 2003年 / 296卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Observations of rich LMC and SMC clusters reveal an increasing spread in core radius (r(c)) with age. This trend likely represents real physical evolution in these systems. Old clusters appear either large or small. Similar r(c) distributions are observed for the Fornax and Sagittarius dSph cluster systems and in the "young" halo Milky Way subsystem. These observations have implications for the formation of the Galaxy and the dynamical evolution of globular clusters.
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页码：497 / 498
页数：2
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