Gravitational quenching by clumpy accretion in cool-core clusters: convective dynamical response to overheating

Keywords

Physics, Astrophysics, Gravitational energy, Cooling flow, Gravitational potential

References

• Turbulent FlowsStephen B. Pope — 2000
• Frontier in astroparticle physics and cosmology : proceedings of the 6th RESCEU International Symposium on D"Frontier in Astroparticle Physics and Cosmology" held on November 4-7, 2003, at the University of Tokyo, Japan勝彦 佐藤, 重博 長瀧 — 2004
• Heat Conduction in Cooling FlowsJoel N. Bregman, L. P. David — 1988
• An X-ray flux-limited sample of clusters of galaxies : evidence for evolution of the luminosity function.A. C. Edge, G. C. Stewart, A. C. Fabian — 1990
• Bursting and quenching in massive galaxies without major mergers or AGNsYuval Birnboim, Avishai Dekel, Eyal Neistein — 2007
• Gravitational quenching in massive galaxies and clusters by clumpy accretionAvishai Dekel, Yuval Birnboim — 2007
• SHAKEN AND STIRRED: CONDUCTION AND TURBULENCE IN CLUSTERS OF GALAXIESM. Ruszkowski, S. Peng Oh — 2009
• Convective and Rotational Stability of a Dilute PlasmaSteven A. Balbus — 2001
• Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational CondensationWilliam H. Press, Paul L. Schechter — 1974
• GRAVITATIONAL HEATING HELPS MAKE MASSIVE GALAXIES RED AND DEADPeter H. Johansson, Thorsten Naab, Jeremiah P. Ostriker — 2009
• Dynamical, physical, and chemical properties of emission-line nebulae in cooling flowsTimothy M. Heckman, Stefi A. Baum, W. J. M. van Breugel — 1989
• The role of heat conduction in the cooling flows of galaxy clustersEdmund Bertschinger, Avery Meiksin — 1986
• ANISOTROPIC THERMAL CONDUCTION AND THE COOLING FLOW PROBLEM IN GALAXY CLUSTERSIan J. Parrish, Eliot Quataert, Prateek Sharma — 2009
• Adding Environmental Gas Physics to the Semianalytic Method for Galaxy Formation: Gravitational HeatingSadegh Khochfar, Jeremiah P. Ostriker — 2007
• On Magnetic Fields, Heating and Thermal Conduction in Halos, and the Suppression of Cooling FlowsR. Rosner, W. H. Tucker — 1989
• Thermal Balance in the Intracluster Medium: Is AGN Feedback Necessary?Charlie Conroy, Jeremiah P. Ostriker — 2007
• Self-similar secondary infall and accretion in an Einstein-de Sitter universeEdmund Bertschinger — 1985
• Dynamical Friction in a Gaseous MediumEve C. Ostriker — 1998
• Galaxy bimodality due to cold flows and shock heatingAvishai Dekel, Yuval Birnboim — 2004
• Measuring the non-thermal pressure in early-type galaxy atmospheres: a comparison of X-ray and optical potential profiles in M87 and NGC 1399E. Churazov, W. Forman, A. Vikhlinin — 2007

Cited by

• The growth of red sequence galaxies in a cosmological hydrodynamic simulationJ. M. Gabor, R. Davé — 2012
• Absorption-line systems in simulated galaxies fed by cold streamsMichele Fumagalli, J. Xavier Prochaska, Daniel Kasen — 2011
• Star Formation And Galaxy Evolution Since Z~2: Results From Multiwavelength SurveysDrew Brisbin — 2014
• Evolution of density profiles in high-z galaxies: compaction and quenching inside-outSandro Tacchella, Avishai Dekel, C. M. Carollo — 2015
• MAGiiCAT III. INTERPRETING SELF-SIMILARITY OF THE CIRCUMGALACTIC MEDIUM WITH VIRIAL MASS USING Mg ii ABSORPTIONChristopher W. Churchill, Sebastian Trujillo-Gomez, Nikole M. Nielsen — 2013
• Properties of gas clumps and gas clumping factor in the intra-cluster mediumF. Vazza, D. Eckert, A. Simionescu — 2012
• THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ⩽ z < 0.8 IN THE DEEP2/AEGIS SURVEYEdmond Cheung, S. M. Faber, David C. Koo — 2012
• Physical Models of Galaxy Formation in a Cosmological FrameworkRachel S. Somerville, Romeel Davé — 2014
• Hot gas in massive haloes drives both mass quenching and environment quenchingJ. M. Gabor, Romeel Davé — 2014
• CONSTRAINING THE STAR FORMATION HISTORIES IN DARK MATTER HALOS. I. CENTRAL GALAXIESXiaohu Yang, H. J. Mo, Frank C. van den Bosch — 2013
• FORMING EARLY-TYPE GALAXIES IN ΛCDM SIMULATIONS. I. ASSEMBLY HISTORIESPeter H. Johansson, Thorsten Naab, Jeremiah P. Ostriker — 2012
• GALAXY MASS, METALLICITY, RADIUS, AND STAR FORMATION RATESDrew Brisbin, Martin Harwit — 2011
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulationsMichaela Hirschmann, Thorsten Naab, Rachel S. Somerville — 2011
• Quenching massive galaxies with on-the-fly feedback in cosmological hydrodynamic simulationsJ. M. Gabor, R. Davé, B. D. Oppenheimer — 2010
• Using Galaxy Pairs to Probe Star Formation During Major Halo MergersPeter Behroozi, Guangtun Zhu, Henry C. Ferguson — 2015
• Magnetic field amplification by shocks in galaxy clusters: application to radio relicsLuigi Iapichino, M. Brüggen — 2012
• The evolution of massive black holes and their spins in their galactic hostsEnrico Barausse — 2012
• AN IN-DEPTH STUDY OF THE ABUNDANCE PATTERN IN THE HOT INTERSTELLAR MEDIUM IN NGC 4649Michael Loewenstein, David Davis — 2012
• The role of penetrating gas streams in setting the dynamical state of galaxy clustersElad Zinger, Avishai Dekel, Yuval Birnboim — 2015
• Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2Moein Mosleh, Sandro Tacchella, Alvio Renzini — 2017

Related papers

• Buoyant bubbles in a cooling intracluster medium I. Hydrodynamic bubblesA. Gardini — 2006
• The effect of mixing on metallicity gradients in the icmM. Brüggen — 2002
• The chemical enrichment of the icm with bepposaxS. De Grandi, S. Molendi — 2001
• Rescuing the intracluster medium of NGC 5813Noam, Soker, Shlomi — 2016
• Radio sources and the evolution of the intracluster mediumDe Young, T. W. Jones — 2006
• Gravo-thermodynamics of the intracluster medium: Negative heat capacity and dilation of cooling time scalesAdi Nusser — 2008
• A gravitational contribution to the cooling flow problemA. C. Fabian — 2003