来就得意 发表于 2025-4-1 05:49:56

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发酵 发表于 2025-4-1 09:25:00

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DRAFT 发表于 2025-4-1 12:06:46

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

强制性 发表于 2025-4-1 14:27:42

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MIR 发表于 2025-4-1 21:36:58

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..

男生戴手铐 发表于 2025-4-2 01:53:45

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