Titlebook: Cooling Flows in Clusters and Galaxies; A. C. Fabian Book 1988 Kluwer Academic Publishers 1988 cosmic ray.cosmology.observatory.quasar.rel

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Properties of Clusters of Galaxies,gers will tend to disrupt cooling flows. I suggest that the recently observed luminous arcs in clusters may be shocks generated by a subcluster merger in a cluster with a cooling flow. The peaked galaxy distributions and radial orbits suggested by recent studies of clusters will lead to a larger num

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A Catalog(UE) of Cooling Flows,tical and systematic error on the derived physical parameters. Of these 106 clusters, 43 have central cooling times < 2 × 10. years and hence are designated ‘cooling flows’. Mass accretion rates range from ~ 1 - 500 M. yr..

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