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Physical properties of emitting plasma near massive black holes: the Broad Line Region
Published online by Cambridge University Press: 01 August 2006
Abstract
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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.
- 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. 383 - 384
- Copyright
- Copyright © International Astronomical Union 2007
References
Griem, H. R. 1997, Principles of Plasma Spectroscopy (Cambridge University Press)CrossRefGoogle Scholar
Ilić, D., Popović, L. Č.Bon, E., Mediavilla, E. G. & Chavushyan, V. H. 2006, MNRAS, 371, 1610CrossRefGoogle Scholar
LaMura, G. Mura, G., Popović, L. Č., Ciroi, S., Rafanelli, P. & Ilić, D. 2006, ApJ submittedGoogle Scholar
Popović, L. Č., Shapovalova, A. I., Chavushyan, V. H., Ilić, D., Burenkov, A. N. & Marcado, A. 2006, astro-ph/0511676Google Scholar
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