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A New Luminosity Effect in QSO Spectra

Published online by Cambridge University Press:  12 April 2016

Michael R. Corbin
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721, USA
Todd A. Boroson
Affiliation:
U.S. Gemini Program, National Optical Astronomy Observatories, P.O. Box 26732, Tucson, AZ 85726, USA

Abstract

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Comparison of the emission-line and continuum parameters of 48 low-redshift QSOs reveals the asymmetry of the C IV λ1549 broad emission line to be strongly correlated with ultraviolet continuum luminosity, such that increasing luminosity produces increasing redward asymmetry. A similar correlation has been found for broad Hβ. Redward profile asymmetries can be modeled as the result of the gravitational redshift of line photons from the very broad-line region (VBLR) by 109–1010M black holes, but blueward profile asymmetries require a competing effect such as electron scattering.

Type
V. Emission Lines, Absorption Lines, the Continuum, and their Relationships
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Boroson, T.A., & Green, R.F. 1992, ApJS, 80, 109.Google Scholar
Brotherton, M.S., Wills, B.J., Francis, P.J., & Steidel, C.C. 1994, ApJ, 430, 495.Google Scholar
Corbin, M.R. 1993 ApJ, 403, L9.CrossRefGoogle Scholar
Corbin, M.R. 1995, ApJ, 447, 496.Google Scholar
Ferrara, A., & Pietrini, P. 1993, ApJ, 405, 130.CrossRefGoogle Scholar
Kallman, T.R., & Krolik, J.H. 1986, ApJ, 308, 805.Google Scholar
Koratkar, A.P., & Gaskell, C.M. 1991, ApJ, 370, L61.Google Scholar
Popovic, L.C., Vince, I., Atanackovic-Vukmanovic, O., & Kubicela, A. 1995, A&A, 293, 309.Google Scholar