The XMM Cluster Survey: the interplay between the brightest cluster galaxy and the intracluster medium via AGN feedback
dc.contributor.author | Stott, John P. | en_US |
dc.contributor.author | Hickox, Ryan C. | en_US |
dc.contributor.author | Edge, Alastair C. | en_US |
dc.contributor.author | Collins, Chris A. | en_US |
dc.contributor.author | Hilton, Matt | en_US |
dc.contributor.author | Harrison, Craig D. | en_US |
dc.contributor.author | Romer, A. Kathy | en_US |
dc.contributor.author | Rooney, Philip J. | en_US |
dc.contributor.author | Kay, Scott T. | en_US |
dc.contributor.author | Miller, Christopher J. | en_US |
dc.contributor.author | Sahlén, Martin | en_US |
dc.contributor.author | Lloyd‐davies, Ed J. | en_US |
dc.contributor.author | Mehrtens, Nicola | en_US |
dc.contributor.author | Hoyle, Ben | en_US |
dc.contributor.author | Liddle, Andrew R. | en_US |
dc.contributor.author | Viana, Pedro T. P. | en_US |
dc.contributor.author | McCarthy, Ian G. | en_US |
dc.contributor.author | Schaye, Joop | en_US |
dc.contributor.author | Booth, C. M. | en_US |
dc.date.accessioned | 2012-06-15T14:32:34Z | |
dc.date.available | 2013-07-01T14:33:04Z | en_US |
dc.date.issued | 2012-05-21 | en_US |
dc.identifier.citation | Stott, John P.; Hickox, Ryan C.; Edge, Alastair C.; Collins, Chris A.; Hilton, Matt; Harrison, Craig D.; Romer, A. Kathy; Rooney, Philip J.; Kay, Scott T.; Miller, Christopher J.; Sahlén, Martin ; Lloyd‐davies, Ed J. ; Mehrtens, Nicola; Hoyle, Ben; Liddle, Andrew R.; Viana, Pedro T. P.; McCarthy, Ian G.; Schaye, Joop; Booth, C. M. (2012). "The XMM Cluster Survey: the interplay between the brightest cluster galaxy and the intracluster medium via AGN feedback." Monthly Notices of the Royal Astronomical Society 422(3). <http://hdl.handle.net/2027.42/91324> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/91324 | |
dc.description.abstract | Using a sample of 123 X‐ray clusters and groups drawn from the XMM Cluster Survey first data release, we investigate the interplay between the brightest cluster galaxy (BCG), its black hole and the intracluster/group medium (ICM). It appears that for groups and clusters with a BCG likely to host significant active galactic nuclei (AGN) feedback, gas cooling dominates in those with T X > 2 keV while AGN feedback dominates below. This may be understood through the subunity exponent found in the scaling relation we derive between the BCG mass and cluster mass over the halo mass range 10 13 < M 500 < 10 15 M ⊙ and the lack of correlation between radio luminosity and cluster mass, such that BCG AGN in groups can have relatively more energetic influence on the ICM. The L X – T X relation for systems with the most massive BCGs, or those with BCGs co‐located with the peak of the ICM emission, is steeper than that for those with the least massive and most offset, which instead follows self‐similarity. This is evidence that a combination of central gas cooling and powerful, well fuelled AGN causes the departure of the ICM from pure gravitational heating, with the steepened relation crossing self‐similarity at T X = 2 keV. Importantly, regardless of their black hole mass, BCGs are more likely to host radio‐loud AGN if they are in a massive cluster ( T X ≳ 2 keV) and again co‐located with an effective fuel supply of dense, cooling gas. This demonstrates that the most massive black holes appear to know more about their host cluster than they do about their host galaxy. The results lead us to propose a physically motivated, empirical definition of ‘cluster’ and ‘group’, delineated at 2 keV. | en_US |
dc.publisher | Blackwell Publishing Ltd | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Galaxies: Clusters: Intracluster Medium | en_US |
dc.subject.other | Galaxies: Active | en_US |
dc.subject.other | Galaxies: Elliptical and Lenticular, CD | en_US |
dc.title | The XMM Cluster Survey: the interplay between the brightest cluster galaxy and the intracluster medium via AGN feedback | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | Extragalactic and Cosmology Group, Department of Physics, University of Durham, South Road, Durham DH1 3LE | en_US |
dc.contributor.affiliationother | Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD | en_US |
dc.contributor.affiliationother | School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD | en_US |
dc.contributor.affiliationother | Astronomy Centre, University of Sussex, Falmer, Brighton BN1 9QH | en_US |
dc.contributor.affiliationother | Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL | en_US |
dc.contributor.affiliationother | The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, SE‐106 91 Stockholm, Sweden | en_US |
dc.contributor.affiliationother | Institute of Sciences of the Cosmos (ICCUB) and IEEC, Physics Department, University of Barcelona, Barcelona 08024, Spain | en_US |
dc.contributor.affiliationother | CSIC, Consejo Superior de Investigaciones Cientificas, Serrano 117, Madrid 28006, Spain | en_US |
dc.contributor.affiliationother | Helsinki Institute of Physics, University of Helsinki, PO Box 64, FIN‐00014 Helsinki, Finland | en_US |
dc.contributor.affiliationother | Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150‐762 Porto, Portugal | en_US |
dc.contributor.affiliationother | Departamento de Física e Astronomia da Faculdade de Ciências da Universidade do Porto, Rua do Campo Alegre 687, 4169‐007 Porto, Portugal | en_US |
dc.contributor.affiliationother | Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA | en_US |
dc.contributor.affiliationother | Astrophysics and Space Research Group, School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT | en_US |
dc.contributor.affiliationother | Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, the Netherlands | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/91324/1/j.1365-2966.2012.20764.x.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2012.20764.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
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