TY - JOUR

T1 - The XMM Cluster Survey

T2 - The interplay between the brightest cluster galaxy and the intracluster medium via AGN feedback

AU - Stott, John P.

AU - Hickox, Ryan C.

AU - Edge, Alastair C.

AU - Collins, Chris A.

AU - Hilton, Matt

AU - Harrison, Craig D.

AU - Romer, A. Kathy

AU - Rooney, Philip J.

AU - Kay, Scott T.

AU - Miller, Christopher J.

AU - Sahlén, Martin

AU - Lloyd-Davies, Ed J.

AU - Mehrtens, Nicola

AU - Hoyle, Ben

AU - Liddle, Andrew R.

AU - Viana, Pedro T P

AU - Mccarthy, Ian G.

AU - Schaye, Joop

AU - Booth, C. M.

PY - 2012/5/21

Y1 - 2012/5/21

N2 - 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 > 2keV 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 13 500 <10 15M ⊙ 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= 2keV. 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≳ 2keV) 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 2keV.

AB - 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 > 2keV 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 13 500 <10 15M ⊙ 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= 2keV. 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≳ 2keV) 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 2keV.

KW - Galaxies: active

KW - Galaxies: clusters: intracluster medium

KW - Galaxies: elliptical and lenticular, cD

U2 - 10.1111/j.1365-2966.2012.20764.x

DO - 10.1111/j.1365-2966.2012.20764.x

M3 - Journal article

AN - SCOPUS:84863400983

VL - 422

SP - 2213

EP - 2229

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -