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...
Gespeichert in:
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| Dokumenttyp: | Konferenzschrift |
| Sprache: | Englisch |
| Veröffentlicht: |
Berlin Heidelberg
Springer
2007
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| Schriftenreihe: | Eso Astrophysics Symposia, European Southern Observatory
SpringerLink Bücher |
| Volumes / Articles: | Show Volumes / Articles. |
| DOI: | 10.1007/978-3-540-73484-0 |
| Schlagworte: | |
| Online-Zugang: | 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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| Verfasserangaben: | edited by H. Böhringer ... |
Inhaltsangabe:
- 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
- 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
- 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
- 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
- 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
- Entropy Generation in Merging Galaxy Clusters