Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the Black Hole Mass-Velocity Dispersion Relationship for Active Galactic Nuclei
We calibrate reverberation-based black hole (BH) masses in active galactic nuclei (AGNs) by using the correlation between BH mass, M sub(BH), and bulge/spheroid stellar velocity dispersion, sigma *. We use new measurements of sigma * for six AGNs and published velocity dispersions for 10 others, in...
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Veröffentlicht in: | The Astrophysical journal 2004-11, Vol.615 (2), p.645-651 |
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creator | Onken, Christopher A Ferrarese, Laura Merritt, David Peterson, Bradley M Pogge, Richard W Vestergaard, Marianne Wandel, Amri |
description | We calibrate reverberation-based black hole (BH) masses in active galactic nuclei (AGNs) by using the correlation between BH mass, M sub(BH), and bulge/spheroid stellar velocity dispersion, sigma *. We use new measurements of sigma * for six AGNs and published velocity dispersions for 10 others, in conjunction with improved reverberation-mapping results, to determine the scaling factor required to bring reverberation-based BH masses into agreement with the quiescent galaxy M sub(BH)- sigma * relationship. The scatter in the AGN BH masses is found to be less than a factor of 3. The current observational uncertainties preclude the use of the scaling factor to discriminate between broad-line region models. |
doi_str_mv | 10.1086/424655 |
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II. Calibration of the Black Hole Mass-Velocity Dispersion Relationship for Active Galactic Nuclei</title><title>The Astrophysical journal</title><description>We calibrate reverberation-based black hole (BH) masses in active galactic nuclei (AGNs) by using the correlation between BH mass, M sub(BH), and bulge/spheroid stellar velocity dispersion, sigma *. We use new measurements of sigma * for six AGNs and published velocity dispersions for 10 others, in conjunction with improved reverberation-mapping results, to determine the scaling factor required to bring reverberation-based BH masses into agreement with the quiescent galaxy M sub(BH)- sigma * relationship. The scatter in the AGN BH masses is found to be less than a factor of 3. 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Active or peculiar galaxies, objects, and systems</topic><topic>Stellar systems. Galactic and extragalactic objects and systems. The universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Onken, Christopher A</creatorcontrib><creatorcontrib>Ferrarese, Laura</creatorcontrib><creatorcontrib>Merritt, David</creatorcontrib><creatorcontrib>Peterson, Bradley M</creatorcontrib><creatorcontrib>Pogge, Richard W</creatorcontrib><creatorcontrib>Vestergaard, Marianne</creatorcontrib><creatorcontrib>Wandel, Amri</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Onken, Christopher A</au><au>Ferrarese, Laura</au><au>Merritt, David</au><au>Peterson, Bradley M</au><au>Pogge, Richard W</au><au>Vestergaard, Marianne</au><au>Wandel, Amri</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the Black Hole Mass-Velocity Dispersion Relationship for Active Galactic Nuclei</atitle><jtitle>The Astrophysical journal</jtitle><date>2004-11-10</date><risdate>2004</risdate><volume>615</volume><issue>2</issue><spage>645</spage><epage>651</epage><pages>645-651</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>We calibrate reverberation-based black hole (BH) masses in active galactic nuclei (AGNs) by using the correlation between BH mass, M sub(BH), and bulge/spheroid stellar velocity dispersion, sigma *. We use new measurements of sigma * for six AGNs and published velocity dispersions for 10 others, in conjunction with improved reverberation-mapping results, to determine the scaling factor required to bring reverberation-based BH masses into agreement with the quiescent galaxy M sub(BH)- sigma * relationship. The scatter in the AGN BH masses is found to be less than a factor of 3. 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subjects | Active and peculiar galaxies (including bl lacertae objects, blazars, seyfert galaxies, markarian galaxies, active galactic nuclei) Astronomy Characteristics and properties of external galaxies and extragalactic objects Earth, ocean, space Exact sciences and technology Galactic nuclei (including black holes), circumnuclear matter, and bulges Quasars. Active or peculiar galaxies, objects, and systems Stellar systems. Galactic and extragalactic objects and systems. The universe |
title | Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the Black Hole Mass-Velocity Dispersion Relationship for Active Galactic Nuclei |
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