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    Chapter and Conference Paper

    Exploring Massive Galaxy Clusters: XMM-Newton observations of two morphology unbiased samples at z ∼ 0.2 and z ∼ 0.3

    For the spectral determination of the temperature distribution in galaxy clusters we developed a double background subtraction method, and applied it to 2 morphology unbiased samples of X-ray luminous galaxy c...

    Y.-Y. Zhang, A. Finoguenov, H. Böhringer in Heating versus Cooling in Galaxies and Clu… (2007)

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    Chapter and Conference Paper

    The Gaseous Atmosphere of M87 seen with XMM-Newton

    Known as the closest cooling-core hosting an active nucleus, M87 is among the best candidates for detailed studies of the mechanisms behind the heating versus cooling balance. The deepest XMM-Newton observatio...

    A. Simionescu, H. Böhringer, M. Brüggen in Heating versus Cooling in Galaxies and Clu… (2007)

  3. No Access

    Chapter and Conference Paper

    XMM-Newton Discovery of an X-Ray Filament in Coma

    XMM-Newton observations of the outskirts of the Coma cluster of galaxies confirm the existence of warm X-ray gas claimed previously and provide a robust estimate of its temperature (~ 0.2 keV) and oxygen abund...

    A. Finoguenov, U. G. Briel, J. P. Henry in Soft X-Ray Emission from Clusters of Galax… (2004)