Heating versus Cooling in Galaxies and Clusters of Galaxies

Heating versus Cooling in Galaxies and Clusters of Galaxies
Author: Hans Böhringer
Publisher: Springer Science & Business Media
Total Pages: 453
Release: 2007-09-27
Genre: Science
ISBN: 3540734848

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This volume documents recent developments that have advanced our understanding of the heating and cooling mechanisms in galaxies and galaxy clusters. Chapters detail results from multi-wavelength observations and advances in numerical hydrodynamical simulations. An additional section covers new research findings on feedback and self-regulatory mechanisms during cosmic structure formation in general and in galaxy formation in particular.


Heating versus Cooling in Galaxies and Clusters of Galaxies
Language: en
Pages: 453
Authors: Hans Böhringer
Categories: Science
Type: BOOK - Published: 2007-09-27 - Publisher: Springer Science & Business Media

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This volume documents recent developments that have advanced our understanding of the heating and cooling mechanisms in galaxies and galaxy clusters. Chapters d
Cooling Flows in Clusters and Galaxies
Language: en
Pages: 377
Authors: A.C. Fabian
Categories: Science
Type: BOOK - Published: 2012-12-06 - Publisher: Springer Science & Business Media

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X-ray astronomers discovered the diffuse gas in clusters of galaxies about 20 years ago. It was later realized that the central gas density in some clusters, an
Regulation of Star Formation Amidst Heating and Cooling in Galaxies and Galaxy Clusters
Language: en
Pages: 342
Authors: Sravani Vaddi
Categories: Galaxies
Type: BOOK - Published: 2016 - Publisher:

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"Galaxy clusters are the largest gravitationally bound systems in the Universe and often host the largest galaxies (known as the brightest cluster galaxies (BCG
Cooling Flows in Clusters and Galaxies
Language: en
Pages: 410
Authors: A C Fabian
Categories:
Type: BOOK - Published: 1988-05-31 - Publisher:

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Clusters of Galaxies: Beyond the Thermal View
Language: en
Pages: 418
Authors: Jelle Kaastra
Categories: Science
Type: BOOK - Published: 2008-05-01 - Publisher: Springer Science & Business Media

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The existence of soft excess emission originating from clusters of galaxies, de ned as em- sion detected below 1 keV in excess over the usual thermal emission f