The Intracluster Medium in z > 1 Galaxy Clusters
The Intracluster Medium in z > 1 Galaxy Clusters
复制标题
z > 1 星系团中的星系团内介质
DOI：
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发表时间：
2000
期刊：
影响因子：
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通讯作者：
H. Spinrad
中科院分区：
文献类型：
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作者：
S. Stanford;B. Holden;P. Rosati;P. Tozzi;S. Borgani;P. Eisenhardt;H. Spinrad
The Chandra X-Ray Observatory was used to obtain a 190 ks image of three high-redshift galaxy clusters in one observation. The results of our analysis of these data are reported for the two z > 1 clusters in this Lynx field, which are the most distant known X-ray luminous clusters. Spatially extended X-ray emission was detected from both these clusters, indicating the presence of hot gas in their intracluster media. A fit to the X-ray spectrum of RX J0849+4452 at z = 1.26 yields a temperature of kT = 5.8 keV. Using this temperature and the assumption of an isothermal sphere, the total mass of RX J0849+4452 is found to be 4.0 × 1014 h M☉ within r = 1 h Mpc. The TX for RX J0849+4452 approximately agrees with the expectation based on its Lbol = 3.3 × 1044 ergs s-1 according to the low-redshift LX-TX relation. The very different distributions of X-ray-emitting gas and of the red member galaxies in the two z > 1 clusters, in contrast to the similarity of the optical/IR colors of those galaxies, suggests that the early-type galaxies mostly formed before their host clusters.
