ASCA observations of massive medium-distant clusters of galaxies I. A 1300 and A 1732

被引:7
作者
Pierre, M [1 ]
Matsumoto, H
Tsuru, T
Ebeling, H
Hunstead, R
机构
[1] CEA, DSM, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France
[2] Kyoto Univ, Fac Sci, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan
[3] RIKEN, Cosm Radiat Lab, Wako, Saitama 3510198, Japan
[4] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[5] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 136卷 / 01期
关键词
galaxies; clusters; general; A; 1300; 1732; intergalactic medium; X-rays : galaxies;
D O I
10.1051/aas:1999458
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have selected a sample of 10 medium distant (z similar to 0.1- 0.3) clusters for deep, high-resolution, multiwavelength observations in order to investigate in detail their dynamical state. This paper presents the analysis of the ASCA data for the two sample clusters observed under the ESA time allocation. For A 1300 and A 1732 we find temperatures and metal abundances for the intracluster medium of kT = 11 keV, Z = 0.2 and kT = 6 keV, Z = 0.3 respectively.
引用
收藏
页码:173 / 177
页数:5
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