NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-04-19 T19:11:39 PDT
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For refcode 2012MNRAS.424..224H:
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Copyright by Royal Astronomical Society. 2012MNRAS.424..224H On the hunt for ultramassive black holes in brightest cluster galaxies Hlavacek-Larrondo, J.; Fabian, A. C.; Edge, A. C.; Hogan, M. T. Abstract. We investigate where brightest cluster galaxies (BCGs) sit on the Fundamental Plane of black hole (BH) activity, an established relation between the X-ray luminosity, the radio luminosity and the mass of a BH. Our sample mostly consists of BCGs that lie at the centres of massive, strong cooling flow clusters, therefore requiring extreme mechanical feedback from their central active galactic nucleus (AGN) to offset cooling of the intracluster plasma (L_mech_>10^44^ -10^45^ erg s^-1^). Based on the BH masses derived from the ? and M_BH_ - M_K_ correlations, we find that all of our objects are offset from the plane such that they appear to be less massive than predicted from their X-ray and radio luminosities (to more than a 99 per cent confidence level). For these objects to be consistent with the Fundamental Plane, the ? and M_BH_ - M_K_ correlations therefore seem to underestimate the BH masses of BCGs, on average by a factor of 10. Our results suggest that the standard relationships between BH mass and host galaxy properties no longer hold for these extreme galaxies. Furthermore, our results imply that if these BHs follow the Fundamental Plane, then many of those that lie in massive, strong cool core clusters must be ultramassive with M_BH_ > 10^10^ M_sun_. This rivals the largest BH masses known and has important ramifications for our understanding of the formation and evolution of BHs. Key words: accretion, accretion discs, black hole physics, galaxies: active, galaxies: clusters: general, galaxies: jets, X-rays: galaxies: clusters
Retrieve 18 NED objects in this reference.
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