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Accretion in the broad line region of active galactic nuclei
Published online by Cambridge University Press: 01 August 2006
Abstract
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We modeled the single-peaked Broad Emission Lines (BELs) with two-component model (accretion disk, with surrounding spherical region), comparing it with observational line profiles for a number of Active Galactic Nuclei (AGN). We find that the accretion in the Broad Line Region (BLR) can be present even if the profiles of BELs are single-peaked.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 329 - 330
- Copyright
- Copyright © International Astronomical Union 2007
References
Bon, E., Popović, L. Č., Ilić, D. & Mediavilla, E. G. 2006, New Ast. Rev., 50, 716CrossRefGoogle Scholar
Ilić, D., Popović, L. Č., Bon, E., Mediavilla, E. G. & Chavushyan, V. H. 2006, MNRAS, 371, 1610CrossRefGoogle Scholar
Popović, L. Č., Mediavilla, E. G., Bon, E., Stanić, N. & Kubičela, A. 2003, ApJ, 599, 185CrossRefGoogle Scholar
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