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Hydromagnetic Wind Model for the Broad-Line Region of NGC 5548
Published online by Cambridge University Press: 12 April 2016
Abstract
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
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- Copyright © Astronomical Society of the Pacific 1997
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