J/ApJ/662/808ivo://CDS.VizieR/J/ApJ/662/808doi:10.26093/cds/vizier.16620808CDSLauer T.R.Faber S.M.Richstone D.Gebhardt K.Tremaine S.Postman M.,Dressler A.Aller M.C.Filippenko A.V.Green R.Ho L.C.Kormendy J.,Magorrian J.Pinkney J.2017-12-07T07:26:58Z2009-07-09T03:39:33ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiescatalogsapparent-magnitudegalaxy-kinematicsBlack hole (BH) masses predicted from the M_BH_-sigma relationship conflict with predictions from the M_BH_-L relationship for high-luminosity galaxies, such as brightest cluster galaxies (BCGs). The M_BH_-L relationship predicts that some BCGs may harbor BHs with M_BH_ approaching 10^10^M_{sun}_ while the M_BH_-sigma relationship always predicts M_BH_<3x10^9^M_{sun}_. We argue that the M_BH_-L relationship is a plausible description for galaxies of high luminosity. If the cores in central stellar density are formed by binary BHs, the inner core cusp radius, r{gamma}, may be an independent witness of M_BH_. Using central structural parameters derived from a large sample of early-type galaxies observed by HST, we argue that L is superior to sigma as an indicator of r{gamma}.2007ApJ...662..808Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/662/808CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/440/28 : Brightest Cluster Galaxies velocities (Postman+ 1995)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/662/808https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/662/808http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/662/808https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/662/808https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/662/808http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/662/808GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJ/662/808/table1Galaxy ParametersNameGalaxy namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMTypeMorphology (1)src.morphcharVMAGAbsolute V band magnitude (2)magphys.magAbs;em.opt.Vfloatsigma? Hyperleda database velocity dispersionkm/sphys.veloc.dispersionintnullablePProfile type (3)meta.code;src.morphcharlogRLog of the cusp radius (4)log(pc)phys.size.radiusfloatmuThe V band cusp surface brightnessmag.arcsec**-2phot.mag.sb;em.opt.VfloatONameAlternative identificationmeta.idcharSimbadNameSimbad column added by the CDSmeta.idcharNEDSimbad column added by the CDSchar