Dynamics of the x-ray clusters Abell 222, Abell 223, Abell 520 and Abell 521

被引：0
|
作者：
Proust, D [1 ]
机构：
[1] Observ Paris, DAEC, Sect Meudon, F-92195 Meudon, France
来源：
DEEP FIELDS | 2001年
关键词：
D O I：
10.1007/10854354_58
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the results of a dynamical analysis as well as the population content of four rich, X-ray luminous galaxy clusters. The detailed observations and analyses can be found in Proust et al (2000) [2] for A222, A223 and A520, and in Maurogordato et al (2000) [1] for A521.
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页码：213 / 213
页数：1
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