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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https://doi.org/10.1007/978-94-009-2953-1cosmic ray; cosmology; observatory; quasar; relativistic jet; star; star formation

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978-94-010-7828-3Kluwer Academic Publishers 1988

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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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ifficult or impossible to reproduce the observed temperature gradient while also reducing the net rate at which cooled gas is produced. None of the models examined lead to a viable alternative cooling flow scenario.

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