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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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樓主: 爆發(fā)
21#
發(fā)表于 2025-3-25 06:17:38 | 只看該作者
Imaging the Hot Intracluster Medium,er virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and scale of cluster substructure can be determined.
22#
發(fā)表于 2025-3-25 09:53:21 | 只看該作者
Large-Scale Structure within Ten Thousand km/s,d (M) 49, 58, 59, 60, 61, 84, 85, 86, 87, 88, 89, 90 & 91. All these nebulae appear to have no stars. They can be seen only in a very clear sky when they are close to the meridian. Most of these nebulae were given me by M. Mechain”.
23#
發(fā)表于 2025-3-25 12:23:43 | 只看該作者
Clusters and Superclusters of Galaxies978-94-011-2482-9Series ISSN 1389-2185
24#
發(fā)表于 2025-3-25 15:54:41 | 只看該作者
Zur Synthese von Antriebssystemen,g on the territory of later speakers, I shall limit myself to general and tentative remarks. I shall try to focus on what we can learn about the origin of clusters and superclusters, emphasising that almost all the observations to be discussed at this meeting are relevant to this issue.
25#
發(fā)表于 2025-3-25 20:23:33 | 只看該作者
26#
發(fā)表于 2025-3-26 00:52:32 | 只看該作者
Schwingungen mechanischer Antriebssystemeer virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and scale of cluster substructure can be determined.
27#
發(fā)表于 2025-3-26 08:18:35 | 只看該作者
28#
發(fā)表于 2025-3-26 09:10:02 | 只看該作者
29#
發(fā)表于 2025-3-26 13:23:08 | 只看該作者
X-Ray Evolution of Clusters of Galaxies,I review the evidence for the evolution of the X-ray luminosity of clusters of galaxies with cosmic epoch. Such evolution has been found in two independent studies. I discuss the constraints that this evolution places on the primordial density fluctuation spectrum.
30#
發(fā)表于 2025-3-26 20:18:20 | 只看該作者
Nato Science Series C:http://image.papertrans.cn/c/image/228561.jpg
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