Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/95
Title: Physical properties of emitting plasma near massive black holes: The Broad Line Region
Authors: Ilić, Dragana 
La Mura, G.
Popovi, L. Ĉ
Shapovalova, A. I.
Ciroi, S.
Chavushyan, V. H.
Rafanelli, P.
Burenkov, A. N.
Marcado, A.
Affiliations: Astronomy 
Keywords: (galaxies:) quasars: emission lines;Galaxies: active;Galaxies: Seyfert
Issue Date: 1-Aug-2006
Related Publication(s): Black Holes from Stars to Galaxies – Across the Range of Masses
Journal: Proceedings of the International Astronomical Union
Abstract: 
We apply the Boltzmann-Plot (BP) method to the Balmer lines to estimate the physical propertiesin the Broad Line Region of Active Galactic Nuclei. We study the Balmer lines of a sample of 90 AGN from Sloan Digital Sky Survey database, as well as the time variability of the BP parameter A of NGC 5548. © 2007 International Astronomical Union.
URI: https://research.matf.bg.ac.rs/handle/123456789/95
ISSN: 17439213
DOI: 10.1017/S174392130700556X
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