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The top documents tagged [cooling flow model]
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INTRODUZIONE A: Aloni radio Ammassi di galassie con e senza cool core
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GH2005 Gas Dynamics in Clusters II Craig Sarazin Dept. of Astronomy University of Virginia A85 Chandra (X-ray) Cluster Merger Simulation
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X-ray Spectroscopy of Accreting White Dwarf Binaries Koji Mukai (NASA/GSFC/CRESST & UMBC)
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GH2005 Gas Dynamics in Clusters II
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Galaxy clusters are the most massive (M~10 14 -10 15 M SUN ) objects in the Universe AN INTRODUCTION TO MERGING GALAXY CLUSTERS Galaxies (5%)Intra-cluster
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