CaltechAUTHORS
Published 1997 | Version public
Book Section - Chapter Metadata-only

Reverberation Modeling of the Broad Emission Line Region in NGC 5548

Creators

  • 1. ROR icon University of Kentucky
  • 2. ROR icon California Institute of Technology

Contributors

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

Identifiers

Eprint ID
96161
Resolver ID
CaltechAUTHORS:20190605-140847085

Dates

Created
2019-06-06
Created from EPrint's datestamp field
Updated
2021-11-16
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Caltech Custom Metadata

Caltech groups
TAPIR
Series Name
Astrophysics and Space Science Library
Series Volume or Issue Number
218