1E 0657-56: A contender for the hottest known cluster of galaxies

被引:97
作者
Tucker, W
Blanco, P
Rappoport, S
David, L
Fabricant, D
Falco, EE
Forman, W
Dressler, A
Ramella, M
机构
[1] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] Carnegie Inst Washington Observ, Pasadena, CA 91101 USA
[4] Osservatorio Astron Trieste, I-34131 Trieste, Italy
基金
美国国家航空航天局;
关键词
galaxies; clusters; individual; (1E; 0657-56); intergalactic medium large-scale structure of universe; X-rays;
D O I
10.1086/311234
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We identify the extended Einstein LPC X-ray source 1E 0657-56 with a previously unknown cluster of galaxies at a redshift of z = 0.296. Optical CCD images show the presence of a gravitational are in this cluster, and galaxy spectra yield a cluster velocity dispersion of 1213(-191)(+352) km s(-1). X-ray data obtained with the ROSAT HRI and ASCA indicate that 1E 0657-56 is a highly luminous cluster in which a merger of subclusters may be occurring. The temperature of the hot gas in 1E 0657-56 is kT = 17.4 +/- 2.5 keV, which makes it an unusually hot cluster, with important cosmological implications.
引用
收藏
页码:L5 / L8
页数:4
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