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

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 rese...

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Bibliographic Details
Other Authors: Böhringer, Hans (Editor)
Format: Conference Paper
Language:English
Published: Berlin Heidelberg Springer 2007
Series:Eso Astrophysics Symposia, European Southern Observatory
SpringerLink Bücher
Volumes / Articles: Show Volumes / Articles.
DOI:10.1007/978-3-540-73484-0
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Online Access:Verlag, Volltext: https://doi.org/10.1007/978-3-540-73484-0
Resolving-System, Volltext: http://dx.doi.org/10.1007/978-3-540-73484-0
Cover: https://swbplus.bsz-bw.de/bsz276337158cov.jpg
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Author Notes:edited by H. Böhringer ...

MARC

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505 8 |a Front Matter; Introduction to Cluster Cooling Cores; Star Formation and Feedback in Cooling Flows; Cold Gas in Cluster Cores; Statistics of X-ray Observables of Cooling Core and Non-cooling Core Clusters of Galaxies; Cold Fronts in Cool Core Clusters; Core structure of Intracluster Gas: Effects of Radiative Cooling on Core Sizes; Investigating the Central Regions of the HIFLUGCS Clusters with Chandra; Investigating Heating and Cooling within a Sample of Distant Clusters; Lack of Cooling Flow Clusters at z > 0.5; The XDCP Prospects of Finding Cooling Core Clusters at Large Lookback Times 
505 8 |a An XMM-Newton View of Three Clusters of GalaxiesExploring Massive Galaxy Clusters: XMM-Newton observations of two morphology unbiased samples at z ~ 0.2 and z ~ 0.3; Heating and Cooling in the Perseus Cluster Core; Hard X-ray emission from the core of the Perseus cluster and the thermal content of the radio bubbles; Outbursts from Supermassive Black Holes: Shocks, Bubbles, and Filaments Around M87; The Gaseous Atmosphere of M87 seen with XMM-Newton; The XMM-Newton View of MS0735+7421: the Most Energetic AGN Outburst in a Galaxy Cluster; Shock Heating by Nearby AGN 
505 8 |a Radio Source Heating in the ICM: The Example of Cygnus AA Deep Chandra Observation of A2052; Chandra and XMM-Newton Observations of the Group of Galaxies HCG 62; Radio Properties of Cavities in the ICM: Imprints of AGN Activity; The Growth of Black Holes and Bulges at the Cores of Cooling Flows; Tracing Ghost Cavities with Low Frequency Radio Observations; High Sensitivity Low Frequency Radio Observations of cD Galaxies; Radio Galaxies in Cooling Cores: Insights from a Complete Sample; Supernova Feedback in Groups and Low-Mass Clusters of Galaxies; Cooling and Feedback in Galaxies and Groups 
505 8 |a Morphological Signatures of AGN Feedback in the Hot Interstellar Medium of Normal Elliptical GalaxiesThermal Structure of the Hot ISM in Normal Ellipticals: Evidence for Local and Distributed AGN Heating; Radio-Loud AGN Heating in Elliptical Galaxies and Clusters; "Radio-active" Brightest Cluster Galaxies; Review of heating mechanisms in clusters of galaxies; Simulating the AGN-ICM Interaction; Simulations of Jets in Dynamic Galaxy Cluster Atmospheres; Can AGN and Radio Sources Reheat the Intracluster Medium?; AGN Heating Through Cavities and Shocks 
505 8 |a The Difficulty of the Heating of Cluster Cooling Flows by Sound Waves and Weak ShocksThe Lifecycle of Powerful AGN Outflows; MHD Simulations of Clusters of Galaxies Including Radiative Cooling; Quantifying "Feedback" in Cool Core and Non-Cool Core Clusters; Buoyant Bubbles in the Virgo Cluster; The Role of AGN Feedback and Gas Viscosity in Hydrodynamical Simulations of Galaxy Clusters; Cold Feedback in Cooling-Flow Galaxy Clusters; AGN Heating of Cooling Flow Clusters: Problems with 3D Hydrodynamic Models; Heating Rate Profiles in Galaxy Clusters; Heating, Cooling, and Intracluster Entropy 
505 8 |a Entropy Generation in Merging Galaxy Clusters 
520 |a 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. 
520 |a 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. 
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