值得尊敬
发表于 2025-3-28 14:54:03
Properties of Clusters of Galaxies,hich the cooling flow environment, which appears to be ubiquitous in the early-type galactic systems which form the hosts for strong radio sources, may affect the origin and structure of the radio emitting regions.
四溢
发表于 2025-3-28 21:32:49
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卧虎藏龙
发表于 2025-3-29 02:04:52
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锡箔纸
发表于 2025-3-29 03:31:00
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苦笑
发表于 2025-3-29 07:33:55
Book 1988usters, and in elliptical galaxies, is so high that radiative cooling is a significant energy loss. The cooling time of the gas decreases rapidly towards the centre of the cluster or galaxy and is less than a Hubble time within the innermost few hundred kiloparsecs. This results in a cooling flow in
grovel
发表于 2025-3-29 14:47:21
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Largess
发表于 2025-3-29 19:17:31
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FLAT
发表于 2025-3-29 21:22:12
Dynamics of Cosmic Rays in Cooling Flows,s interaction by means of steady models with spherical symmetry. It was found that the cosmic ray pressure may become comparable to the gas pressure in the halo region around a central galaxy with a cooling flow. Rayleigh Taylor instabilities might develop there and set the scale for inhomogeneities leading to filaments or star formation regions.
engender
发表于 2025-3-30 01:28:40
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Minuet
发表于 2025-3-30 08:08:08
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