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Hydromagnetic Wind Model for the Broad-Line Region of NGC 5548

Published online by Cambridge University Press:  12 April 2016

M.C. Bottorff ,
K.T. Korista ,
I. Shlosman  and
R.D. Blandford
M.C. Bottorff
Affiliation:
Department of Physics and Astronomy, University of Kentucky, Lexington, KY 40506, USA
K.T. Korista
Affiliation:
Department of Physics and Astronomy, University of Kentucky, Lexington, KY 40506, USA
I. Shlosman
Affiliation:
Department of Physics and Astronomy, University of Kentucky, Lexington, KY 40506, USA
R.D. Blandford
Affiliation:
Theoretical Astrophysics, 130-33, Caltech, Pasadena, CA 91125, USA

Abstract

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A hydromagnetic wind model from a dusty molecular disk (Emmering, Blandford, & Shlosman 1992) was applied to the BLR in NGC 5548 and produced synthetic C IV line profiles as a function of time. The model C IV profiles are compared to data from the 1993 IUE/HST campaign and properties of the the BLR of NGC 5548 are inferred.

Type
IV. Physics of the Broad-Line Region
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 215 - 216
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Bottorff, M., Korista, K., Shlosman, I. & Blandford, R. 1996, ApJ, submitted.Google Scholar
Emmering, R.T., Blandford, R.D. & Shlosman, I. 1992, ApJ, 385, 460.CrossRefGoogle Scholar
Korista, K.T., et al. 1995, ApJS, 97, 285.Google Scholar
Walter, R., et al. 1994, A&A, 285, 119.Google Scholar