SIMBAD references

2018MNRAS.474.1342M - Mon. Not. R. Astron. Soc., 474, 1342-1360 (2018)

The most massive black holes on the Fundamental Plane of black hole accretion.

MEZCUA M., HLAVACEK-LARRONDO J., LUCEY J.R., HOGAN M.T., EDGE A.C. and McNAMARA B.R.

Abstract (from CDS):

We perform a detailed study of the location of brightest cluster galaxies (BCGs) on the Fundamental Plane of black hole (BH) accretion, which is an empirical correlation between a BH X-ray and radio luminosity and mass supported by theoretical models of accretion. The sample comprises 72 BCGs out to z ∼ 0.3 and with reliable nuclear X-ray and radio luminosities. These are found to correlate as LX ∝LR^0.75 ±0.08^, favouring an advection-dominated accretion flow as the origin of the X-ray emission. BCGs are found to be on average offset from the Fundamental Plane such that their BH masses seem to be underestimated by the MBH-MK relation a factor ∼10. The offset is not explained by jet synchrotron cooling and is independent of emission process or amount of cluster gas cooling. Those core-dominated BCGs are found to be more significantly offset than those with weak core radio emission. For BCGs to on average follow the Fundamental Plane, a large fraction ( ∼ 40 per cent) should have BH masses >1010 M and thus host ultramassive BHs. The local BH-galaxy scaling relations would not hold for these extreme objects. The possible explanations for their formation, either via a two-phase process (the BH formed first, the galaxy grows later) or as descendants of high-z seed BHs, challenge the current paradigm of a synchronized galaxy-BH growth.

Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): accretion, accretion discs - black hole physics - galaxies: active - galaxies: clusters: general - galaxies: jets - X-rays: galaxies: clusters

Status in Simbad:  being processed

Simbad objects: 104

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2019.07.19-11:14:49

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