Published 1997
| public
Book Section - Chapter
Reverberation Modeling of the Broad Emission Line Region in NGC 5548
Chicago
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Abstract
Long-term observations of broad-line region (BLR) in the Seyfert 1 galaxy NGC 5548 are analyzed and compared with the predictions of the hydromagnetically driven outflow model of Emmering, Blandford and Shlosman Here we use the model to compute the delay between the C IV line and the continuum. We show, by use of the two-dimensional transfer function (2DTF), that the model predicts a red-side-first-response for the emission line.
Additional Information
© 1997 Springer Science+Business Media Dordrecht.Additional details
- Eprint ID
- 96161
- Resolver ID
- CaltechAUTHORS:20190605-140847085
- Created
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2019-06-06Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Caltech groups
- TAPIR
- Series Name
- Astrophysics and Space Science Library
- Series Volume or Issue Number
- 218