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Titlebook: Clusters and Superclusters of Galaxies; A. C. Fabian Book 1992 Springer Science+Business Media Dordrecht 1992 Galaxy.Gravity.Quasar.Univer

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楼主: 爆发
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https://doi.org/10.1007/978-3-663-05570-9red luminosity toward the cD galaxies in rich clusters..Stellar mass loss from galaxies and radiative cooling by dust could produce cool cluster gas at a rate approaching 1000 M./yr unless balanced by a heating mechanism. Thermal electron conduction can be an effective heating agent and we examine w
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https://doi.org/10.1007/978-3-662-09835-6source required to maintain the ionization of the gas. The physical properties of the nebulae are presented, the difficulties posed by the nebulae for the standard cooling flow scenario are discussed, and possible sources for the origin and ionization of the gas are explored. The evidence points to
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Einfache lineare Schwingungssysteme,erclusters, following recent developments on the scaling properties of galaxies at large separations. Finally, we look at the interplay between galaxy morphology and luminosity on one side, and the supercluster environment (local density) on the other. We discuss recent evidences showing that galaxi
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Bodenkräfte einer Rüttelmaschine products of this rapid evolution of quasars in rich clusters are radio galaxies in rich clusters at low redshift. By combining data from quasars and low-redshift radio galaxies, it is shown that they can both be consistently described by a single luminosity function and evolution law. Possible expl
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Bodenkräfte einer Rüttelmaschineer epoch by non-gravitational processes. If one discards the optical observations, an alternative is to invoke primordial fluctuations with a much redder spectrum, and I discuss how one might discriminate between these theories with future observations.
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