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X-Ray Evolution of Clusters of Galaxies
1992I review the evidence for the evolution of the X-ray luminosity of clusters of galaxies with cosmic epoch. Such evolution has been found in two independent studies. I discuss the constraints that this evolution places on the primordial density fluctuation spectrum.
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X-Ray Spectra of Clusters of Galaxies
1981X-ray spectroscopy has played a crucial role in the study of clusters of galaxies, possibly more so than in any other area. In one stroke, the detection of iron line emission from clusters by Mitchell et al. (1976) and Serlemitsos et al. (1977) showed that the dominant X-ray emission mechanism is thermal bremsstrahlung and that the intracluster gas is ...
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X-Ray Spectroscopy of Galaxy Clusters
1994In the past few years, the results obtained with the X-ray satellites EXOSAT and GlNGA, combined with more ancient data from the EINSTEIN satellite (SSS and MPC), have greatly increased our knowledge of the spectroscopic properties of the intra-cluster medium.
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X-ray Observations of Clusters of Galaxies
1988Because Sarazin (1986) has written a very extensive review of the x-ray emission from clusters of galaxies I have allowed myself considerable leeway in writing this review. In particular it has allowed me to be incomplete in my references and to omit certain topics.
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The X-Ray View of Galaxy Clusters
2005Clusters of galaxies are the most massive collapsed systems in the Universe. A typical luminous cluster (e.g., Coma cluster) is filled with a hot, 100 million degree, low density (10−3 cm−3) gas. In addition to the optically luminous galaxies and diffuse X-ray gas, clusters are dominated by dark matter.
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