The luminous material in clusters of galaxies falls primarily into two forms: the visible galaxies and the X-ray emitting intracluster medium. The hot intracluster medium is the major observed baryonic component of clusters with a mass equal to or greater than that of the stellar matter. In this paper, the structure and morphology of rich clusters as inferred from X-ray observations of the ICM are reviewed. Changes in the efficiency of galaxy formation for different clusters and the origin of the intracluster medium are also discussed.


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    Titel :

    Clusters of galaxies and the hot intracluster medium


    Beteiligte:
    Jones, C. (Autor:in) / Forman, W. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1990-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Clusters of galaxies and the hot intracluster medium

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    A Two-Temperature Model of the Intracluster Medium

    Takizawa, M. / International Council of Scientific Unions | British Library Conference Proceedings | 2000


    The Interaction between the Central Galaxy and the Intracluster Medium in Cool Cluster Cores

    Hatch, N. A. / Crawford, C. S. / Fabian, A. C. et al. | British Library Conference Proceedings | 2005