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• W1644941013 startingPage "647" @default.
• W1644941013 abstract "It has been proposed that the width of the narrow [O III] λ5007 emission line can be used as a surrogate for the stellar velocity dispersion in active galaxies. This proposition is tested using the Sloan Digital Sky Survey (SDSS) Early Data Release (EDR) spectra of 107 low-redshift radio-quiet QSOs and Seyfert 1 galaxies by investigating the correlation between black hole mass, as determined from Hβ 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." @default.
• W1644941013 created "2016-06-24" @default.
• W1644941013 creator A5044802181 @default.
• W1644941013 date "2003-03-10" @default.
• W1644941013 modified "2023-09-25" @default.
• W1644941013 title "Does the Narrow [O<scp>iii</scp>] λ5007 Line Reflect the Stellar Velocity Dispersion in Active Galactic Nuclei?" @default.
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• W1644941013 doi "https://doi.org/10.1086/346111" @default.
• W1644941013 hasPublicationYear "2003" @default.
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