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ASCA Observations of Distant Clusters of Galaxies

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The Hot Universe

Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 188))

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Abstract

Investigation of evolution of X-ray properties of clusters of galaxies is a key study of cosmology. The most important result in this field before ROSAT and ASCA observatories is the detection of the negative evolution of the X-ray luminosity function at red-shift lower than 0.6 (Gioia et al., 1990). Following it, many groups have been investigating evolution of X-ray luminosity function from various surveys with ROSAT observatory (eg. Collins et al., 1997). Many of them indicate no negative evolution at the red-shift lower than 0.7, which is against the Einstein result.

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© 1998 Springer Science+Business Media Dordrecht

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Tsuru, T.G. (1998). ASCA Observations of Distant Clusters of Galaxies. In: Koyama, K., Kitamoto, S., Itoh, M. (eds) The Hot Universe. International Astronomical Union / Union Astronomique Internationale, vol 188. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4970-9_15

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  • DOI: https://doi.org/10.1007/978-94-011-4970-9_15

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-5059-0

  • Online ISBN: 978-94-011-4970-9

  • eBook Packages: Springer Book Archive

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