The host galaxies of luminous quasars

Show simple item record

dc.contributor.author Floyd, David en_US
dc.contributor.author Kukula, Marek en_US
dc.contributor.author Dunlop, James en_US
dc.contributor.author McLure, Ross en_US
dc.contributor.author Miller, Lance en_US
dc.contributor.author Percival, Will en_US
dc.contributor.author Baum, Stefi en_US
dc.contributor.author O'Dea, Christopher en_US
dc.date.accessioned 2006-05-11T17:23:05Z en_US
dc.date.available 2006-05-11T17:23:05Z en_US
dc.date.issued 2004-11 en_US
dc.identifier.citation Mon.Not.Roy.Astron.Soc. 355 (2004) 196-220 en_US
dc.identifier.issn 1365-2966 en_US
dc.identifier.uri http://hdl.handle.net/1850/1788 en_US
dc.description RIT community members may access full-text via RIT Libraries licensed databases: http://library.rit.edu/databases/
dc.description.abstract We present the results of a deep HST/WFPC2 imaging study of 17 quasars at z~=0.4, designed to determine the properties of their host galaxies. The sample consists of quasars with absolute magnitudes in the range −24 ≥ MV ≥ −28, allowing us to investigate host galaxy properties across a decade in quasar luminosity, but at a single redshift. Our previous imaging studies of AGN hosts have focussed primarily on quasars of moderate luminosity, but the most powerful objects in the current sample have powers comparable to the most luminous quasars found at high redshifts. We find that the host galaxies of all the radio-loud quasars, and all the radio- quiet quasars in our sample with nuclear luminosities MV < −24, are massive bulge- dominated galaxies, confirming and extending the trends deduced from our previous studies. From the best-fitting model host galaxies we have estimated spheroid and hence black-hole masses, and the efficiency (with respect to the Eddington luminosity) with which each quasar is emitting radiation. The largest inferred black-hole mass in our sample is MBH~=3×10^9M⊙, comparable to the mass of the black-holes at the centres of M87 and Cygnus A. We find no evidence for super-Eddington accretion rates in even the most luminous objects (0.05 < L/LEdd < 1.0). We investigate the role of scatter in the black-hole:spheroid mass relation in determining the ratio of quasar to host-galaxy luminosity, by generating simulated populations of quasars lying in hosts with a Schechter mass function. Within the subsample of the highest-luminosity quasars, the observed variation in nuclear-host luminosity ratio is consistent with being the result of the scatter in the black-hole:spheroid relation. Quasars with high nuclear-host luminosity ratios can be explained in terms of sub-Eddington accretion rates onto black-holes in the high-mass tail of the black-hole:spheroid relation. Our results imply that, owing to the Schechter function cutoff, host mass should not continue to increase linearly with quasar luminosity, at the very highest luminosities. Any quasars more luminous than MV=−27 should be found in massive elliptical hosts which at the present day would have MV~=−24.5 (Refer to PDF file for exact formulas). en_US
dc.description.sponsorship Based on observations with the NASA/ESA Hubble Space Telescope, (program ID’s 7447 and 8609) obtained at the Space Telescope Science Institute, which is operated by The Association of Universities for Research in Astronomy, Inc. under NASA contract No. NAS5-26555. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. James Dunlop acknowledges the enhanced research time afforded by the award of a PPARC Senior Fellowship. DJEF, MJK, RJM & WJP also acknowledge PPARC funding. We thank the anoymous referee for a fair and constructive critique which has led to significant improvements in this paper. en_US
dc.format.extent 434441 bytes en_US
dc.format.mimetype application/pdf en_US
dc.language.iso en_US en_US
dc.publisher Blackwell Publishing en_US
dc.relation.ispartofseries vol. 355 en_US
dc.relation.ispartofseries no. 1 en_US
dc.subject Black hole physics en_US
dc.subject Galaxies - active en_US
dc.subject Galaxies - evolution en_US
dc.subject Quasars - general en_US
dc.title The host galaxies of luminous quasars en_US
dc.type Article en_US
dc.identifier.url http://dx.doi.org/10.1111/j.1365-2966.2004.08315.x

Files in this item

Files Size Format View

An open access version of this file is not available. Check "Publisher URL" field for access

This item appears in the following Collection(s)

Show simple item record

Search RIT DML


Advanced Search

Browse