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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)
51#
發(fā)表于 2025-3-30 10:15:57 | 只看該作者
52#
發(fā)表于 2025-3-30 16:11:20 | 只看該作者
53#
發(fā)表于 2025-3-30 17:28:37 | 只看該作者
Rosat Observations of Clusters of Galaxies,h photon yield in the survey like Virgo, Perseus, nad AWM7 are presented to illustrate the capabilities of ROSAT in galaxy cluster studies. In addition we discuss the prospects for detections of clusters of galaxies in the All Sky Survey and their possible implication for cosmological research.
54#
發(fā)表于 2025-3-31 00:44:27 | 只看該作者
,X—Ray Spectral Images of Clusters, spatially resolved spectroscopy and present preliminary BBXRT results on several clusters. The BBXRT results are in good agreement with simple cooling flow theory, in 3 cases confirm the existence of cold material in the cluster, find only shallow abundance gradients and constrain the mass profile in the central regions of the cluster.
55#
發(fā)表于 2025-3-31 01:44:54 | 只看該作者
,The Sunyaev—Zeldovich Effect,role in elucidating cluster physics, its relationship to other microwave background anisotropies, and the prospects for improved measurements of both its amplitude and two-dimensional structure via a new generation of instruments.
56#
發(fā)表于 2025-3-31 06:45:30 | 只看該作者
57#
發(fā)表于 2025-3-31 13:11:53 | 只看該作者
Book 1992stitute held inCambridge, England in July 1991. .Much of the material is presented in a pedagogical manner and willappeal to scientists, astronomers and graduate students interested inextragalactic astronomy. .
58#
發(fā)表于 2025-3-31 14:39:22 | 只看該作者
59#
發(fā)表于 2025-3-31 20:17:51 | 只看該作者
60#
發(fā)表于 2025-4-1 00:50:06 | 只看該作者
Schwingungen mechanischer Antriebssysteme spatially resolved spectroscopy and present preliminary BBXRT results on several clusters. The BBXRT results are in good agreement with simple cooling flow theory, in 3 cases confirm the existence of cold material in the cluster, find only shallow abundance gradients and constrain the mass profile in the central regions of the cluster.
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