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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...
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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...
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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...