Heating versus Cooling in Galaxies and Clusters of Galaxies : Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006

Language: English

Published by Springer, 2007

354073483X / 9783540734833

Series: Book 11 of 12 - ESO Astrophysics Symposia

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Druck auf Anfrage Neuware - Printed after ordering - The Universe would be a dull and dark place if the gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e ciency, so that far more than the observed fraction of about 10-15% of the baryonic matter would be found in luminous stellar systems. Therefore,cooling must be damped or regulatedby heating processes, and observations show that this 'feedback' is a widespread astrophysical phenomenon. The place where this cooling and feedback manifests itself most dram- ically is in the inner regions of the most massive Dark Matter halos found in our Universe, in the cores of galaxy clusters. The e ect of cosmic co- ing in these objects was recognized in the mid-1970s, and the term 'cooling ow' was introduced by Andy Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causing an in ow of hot gas from larger radii.…

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Title
Heating versus Cooling in Galaxies and Clusters of Galaxies : Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006
Author
Alexis Finoguenov
Publisher
Springer
Publication year
2007
Condition
Neu
Binding
Buch
Language
English
ISBN 10
354073483X
ISBN 13
9783540734833
Item weight
818 grams
Dimensions
241x160x31 mm
Series
Book 11 of 12: ESO Astrophysics Symposia

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