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Heating versus Cooling in Galaxies and Clusters of Galaxies - H. Böhringer#G.W. Pratt#A. Finoguenov#P. Schuecker
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H. Böhringer#G.W. Pratt#A. Finoguenov#P. Schuecker:

Heating versus Cooling in Galaxies and Clusters of Galaxies - neues Buch

2007, ISBN: 9783540734833

ID: 691814043

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 1015% 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. Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006 Bücher > Fremdsprachige Bücher > Englische Bücher gebundene Ausgabe 02.11.2007, Springer, .200

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Heating versus Cooling in Galaxies and Clusters of Galaxies - H. Böhringer#G.W. Pratt#A. Finoguenov#P. Schuecker
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H. Böhringer#G.W. Pratt#A. Finoguenov#P. Schuecker:

Heating versus Cooling in Galaxies and Clusters of Galaxies - neues Buch

2006, ISBN: 9783540734833

ID: e1a129f231950229fec2136b5cded373

Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006 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 1015% 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. Bücher / Fremdsprachige Bücher / Englische Bücher 978-3-540-73483-3, Springer

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Heating Versus Cooling in Galaxies and Clusters of Galaxies - Pratt, Gabriel W.; Schucker, Peter; Bohringer, Hans; Finoguenov, Alexis A.
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Pratt, Gabriel W.; Schucker, Peter; Bohringer, Hans; Finoguenov, Alexis A.:
Heating Versus Cooling in Galaxies and Clusters of Galaxies - neues Buch

ISBN: 9783540734833

ID: 337887

The present volume is the record of a recent topical conference on the interplay between heating and cooling processes in galaxies and clusters of galaxies. The volume documents recent progress in our understanding of the dense central regions of these objects. Chapters detail recent results from multiwavelength observations and advances in numerical hydrodynamical simulations. An additional section covers new research on feedback and self-regulatory mechanisms during cosmic structure formation in general, and in galaxy formation in particular. With reviews and technical papers written by leading scientists, this state-of-the art report will be a valuable and comprehensive source of reference for all astronomers and astrophysicists active in this field. Science Science eBook, Springer

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Heating Versus Cooling In Galaxies And Clusters Of Galaxies: Proceedings Of The Mpa/Eso/Mpe/Usm Joint Astronomy Conference Held In Garching, - G. W. Pratt, H. Bohringer, A. Finoguenov
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Heating Versus Cooling In Galaxies And Clusters Of Galaxies: Proceedings Of The Mpa/Eso/Mpe/Usm Joint Astronomy Conference Held In Garching, - gebunden oder broschiert

2011, ISBN: 9783540734833

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Heating versus Cooling in Galaxies and Clusters of Galaxies - Hans Böhringer; Gabriel W. Pratt; Alexis Finoguenov; Peter Schuecker
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Hans Böhringer; Gabriel W. Pratt; Alexis Finoguenov; Peter Schuecker:
Heating versus Cooling in Galaxies and Clusters of Galaxies - gebunden oder broschiert

2007, ISBN: 9783540734833

ID: 8192957

Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006, 2007, Hardcover, Buch, [PU: Springer Berlin]

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Heating versus Cooling in Galaxies and Clusters of Galaxies
Autor:

Gabriel W. Pratt

Titel:

Heating versus Cooling in Galaxies and Clusters of Galaxies

ISBN-Nummer:

9783540734833

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.

Detailangaben zum Buch - Heating versus Cooling in Galaxies and Clusters of Galaxies


EAN (ISBN-13): 9783540734833
ISBN (ISBN-10): 354073483X
Gebundene Ausgabe
Erscheinungsjahr: 2007
Herausgeber: Springer-Verlag GmbH
446 Seiten
Gewicht: 0,773 kg
Sprache: eng/Englisch

Buch in der Datenbank seit 10.11.2007 00:07:42
Buch zuletzt gefunden am 26.12.2016 12:47:38
ISBN/EAN: 9783540734833

ISBN - alternative Schreibweisen:
3-540-73483-X, 978-3-540-73483-3

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