The Black Hole-Host Galaxy Relation in Active Galactic Nuclei

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dc.creatorWandel, Amri
dc.date2000-09-21
dc.date.accessioned2026-07-07T01:55:35Z
dc.date.available2026-07-07T01:55:35Z
dc.descriptionThe masses of the central black holes of Active Galactic Nuclei estimated by the reverberation virial technique seem to be significantly smaller than predicted from the black hole mass-bulge luminosity relation for massive black holes detected by kinematic methods in less active and normal galaxies. We reexamine the relation for updated data and suggest a few reasons that may cause this discrepancy.
dc.description10 pages, 2 figures, to appear in "Probing the Physics of AGN by Multiwavelength Monitoring", ASP
dc.identifierhttps://arxiv.org/abs/astro-ph/0009357
dc.identifierhttp://arxiv.org/abs/astro-ph/0009357
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1706
dc.subjectAstrophysics
dc.titleThe Black Hole-Host Galaxy Relation in Active Galactic Nuclei
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