The formation and evolution of massive star clusters: Historical overview

被引：0
|
作者：
van den Bergh, S [1 ]
机构：
[1] Natl Res Council Canada, Herzberg Inst Astrophys, Dominion Astrophys Observ, Victoria, BC V9E 2E7, Canada
来源：
FORMATION AND EVOLUTION OF MASSIVE YOUNG STAR CLUSTERS | 2004年 / 322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：
Some factors connecting the evolutionary histories of galaxies with the characteristics of their cluster systems are reviewed. Unanswered questions include: How is one to understand the observation that some globular cluster systems have disk kinematics whereas others do not? Why do some galaxies have cluster systems with unimodal metallicity distributions, whereas others have bimodal metallicity distributions? What caused the average ellipticity of individual clusters to differ from galaxy to galaxy?
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页码：3 / 8
页数：6
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