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DOI10.1126/science.274.5291.1335
Diffuse extreme-ultraviolet emission from the Coma cluster: Evidence for rapidly cooling gases at submegakelvin temperatures
Lieu R.; Mittaz J.P.D.; Bowyer S.; Breen J.O.; Lockman F.J.; Murphy E.M.; Hwang C.-Y.
发表日期1996
ISSN0036-8075
起始页码1335
结束页码1338
卷号274期号:5291
英文摘要The central region of the Coma cluster of galaxies was observed in the energy band from 0.065 to 0.245 kiloelectron volts by the Deep Survey telescope aboard the Extreme Ultraviolet Explorer. A diffuse emission halo of angular diameter ~30 arc minutes was detected. The extreme-ultraviolet (EUV) emission level exceeds that expected from the x-ray temperature gas in Coma. This hale suggests the presence of two more phases in the emitting gas, one at a temperature of ~2 x 106 kelvin and the other at ~8 x 105 kelvin. The letter phase cools rapidly and, in steady state, would have produced cold matter with a mass of ~1014 solar masses within the EUV halo. Although a similar EUV enhancement was discovered in the Virgo cluster, this detection in Coma applies to a noncooling flow system.
英文关键词article; astronomy; cooling; gas; priority journal; temperature; ultraviolet radiation; X ray
语种英语
来源期刊Science
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/244542
作者单位Department of Physics, University of Alabama, Huntsville, AL 35899, United States; Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom; Ctr. Extreme Ultraviolet Astrophys., University of California, Berkeley, CA 94720, United States; Astronomy Department, University of Virginia, Post Office Box 3818, Charlottesville, VA 22903, United States; National Radio Astronomy Observatory, Green Bank, WV 24944, United States
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Lieu R.,Mittaz J.P.D.,Bowyer S.,et al. Diffuse extreme-ultraviolet emission from the Coma cluster: Evidence for rapidly cooling gases at submegakelvin temperatures[J],1996,274(5291).
APA Lieu R..,Mittaz J.P.D..,Bowyer S..,Breen J.O..,Lockman F.J..,...&Hwang C.-Y..(1996).Diffuse extreme-ultraviolet emission from the Coma cluster: Evidence for rapidly cooling gases at submegakelvin temperatures.Science,274(5291).
MLA Lieu R.,et al."Diffuse extreme-ultraviolet emission from the Coma cluster: Evidence for rapidly cooling gases at submegakelvin temperatures".Science 274.5291(1996).
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