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Preprint 904

Author(s): Boroson, Todd A.
Title: Does the Narrow [O III]\lambda5007 Line Reflect the Stellar Velocity Dispersion in AGN?
Abstract:
It has been proposed that the width of the narrow [O III] \lambda5007 emission line can be used as a surrogate for the stellar velocity dispersion in active galaxies. This proposition is tested using the SDSS EDR spectra of 107 low-redshift radioquiet QSOs and Seyfert 1 galaxies by investigating the correlation between black hole mass, as determined from H\Beta FWHM and optical luminosity, and [O III] FWHM. The correlation is real, but the scatter is large. Without additional information or selection criteria, the [O III] width can predict the black hole mass to a factor of 5.
Date Received: December 02, 2002
Publication Info: ApJ 585:647-652


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