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

爆发

书目名称Clusters and Superclusters of Galaxies影响因子(影响力)




书目名称Clusters and Superclusters of Galaxies影响因子(影响力)学科排名




书目名称Clusters and Superclusters of Galaxies网络公开度




书目名称Clusters and Superclusters of Galaxies网络公开度学科排名




书目名称Clusters and Superclusters of Galaxies被引频次




书目名称Clusters and Superclusters of Galaxies被引频次学科排名




书目名称Clusters and Superclusters of Galaxies年度引用




书目名称Clusters and Superclusters of Galaxies年度引用学科排名




书目名称Clusters and Superclusters of Galaxies读者反馈




书目名称Clusters and Superclusters of Galaxies读者反馈学科排名

生命层

Far Infrared Emission from Clusters and Warming Flows,red 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

prostate-gland

The Intracluster Medium,sion processes and physical properties of the ICM are reviewed. The ICM is probably inhomogeneous, with blobs of denser and cooler gas intermixed with hotter, more diffuse gas. If this is correct, the density fluctuations may complicate eft’orts to use the ICM to determine cluster masses and distanc

亚麻制品

Cooling Flows in Clusters of Galaxies,ations of the ionization state of the optical nebulosity and measurements of Faraday rotation and depolarization of radio lobes show that many luminous radio-loud objects are surrounded by massive cooling flows. They may therefore be an important phase in the formation of the most massive galaxies.

侵略者

骂人有污点

Clusters as Gravitational Lenses, The detection of more than 50 arclets in some rich clusters will enable one to better probe the mass content and the distribution of dark matter in clusters, as well as indications on the redshift distribution of the background galaxies.

骂人有污点

Superclusters and Large-Scale Structure,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

骑师

Galaxy Clusters Around Quasars, 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

ESPY

抱狗不敢前

Schwingungen mechanischer Antriebssystemet in many clusters at both optical and X—ray wavelengths. Although its strength and prevalence are hard to quantify, it clearly causes a nmnber of biases both in cluster definition and in the measurement of cluster properties. I illustrate the problems using clusters selected from simulations of a C