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Reverberation mapping of the emission line regions of Seyfert galaxies and quasars

Blandford, R. D., McKee, C. F.·1982·The Astrophysical Journal

Abstract

An indirect method is outlined for mapping the emission line regions of Seyfert galaxies and quasars having variable line intensities and profiles, provided that (1) the galactic nuclei in question comprise a compact, central continuum source surrounded by an extended distribution of line-emitting gas, and (2) that the covering factor of the gas be small and the entire region optically thin to Thomson scattering so that most continuum and line photons may escape directly from the nucleus. The results obtained are demonstrated by means of models in which the line luminosity of an element of gas is directly proportional to the incident observed continuum flux. Additional assumptions justified on physical grounds are rapid reprocessing and the stability of the gas distribution over several light crossing times.

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Metadata

Authors
Blandford, R. D., & McKee, C. F.
Venue
The Astrophysical Journal
Published
1982-04
Volume
255
Pages
419
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2095424371
Cited by
1,073
References
0
FWCI
0.00
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Reverberation mapping of the emission line regions of Seyfert galaxies and quasars. https://app.cochat.ai/papers/10.1086/159843
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Blandford, R. D., & McKee, C. F. (1982). Reverberation mapping of the emission line regions of Seyfert galaxies and quasars. The Astrophysical Journal. https://doi.org/10.1086/159843

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