音乐会 发表于 2025-3-25 06:58:07

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精美食品 发表于 2025-3-25 07:37:49

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并排上下 发表于 2025-3-25 12:05:48

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

aggravate 发表于 2025-3-25 17:21:55

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

领导权 发表于 2025-3-25 20:03:11

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芦笋 发表于 2025-3-26 00:16:38

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..

CRUE 发表于 2025-3-26 08:22:44

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.

波动 发表于 2025-3-26 09:34:40

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Outshine 发表于 2025-3-26 14:40:20

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是剥皮 发表于 2025-3-26 19:08:56

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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