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    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)