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• W2005202357 abstract "The Broad Emission Lines (BELs) in spectra of type 1 Active Galactic Nuclei (AGN) can be very complex, indicating a complex Broad Line Region (BLR) geometry. According to the standard unification model one can expect an accretion disk around a supermassive black hole in all AGN. Therefore, a disk geometry is expected in the BLR. However, a small fraction of BELs show double-peaked profiles which indicate the disk geometry. Here, we discuss a two-component model, assuming an emission from the accretion disk and one additional emission from surrounding region. We compared the modeled BELs with observed ones (mostly broad H$alpha$ and H$beta$ profiles) finding that the model can well describe single-peaked and double-peaked observed broad line profiles." @default.
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• W2005202357 date "2009-07-01" @default.
• W2005202357 modified "2023-10-03" @default.
• W2005202357 title "Complex broad emission line profiles of AGN – Geometry of the broad line region" @default.
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• W2005202357 doi "https://doi.org/10.1016/j.newar.2009.09.007" @default.
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