Some Spectroscopic Methods for Astrophysical Plasma Research
作者:
L. Cˇ. Popovic´,
M. S. Dimitrijevic´,
E. Mediavilla,
E. Danezis,
E. Lyratzi,
E. Bon,
D. Ilic´,
P. Jovanovic´,
E. Theodossiou,
M. Dacˇic´,
期刊:
AIP Conference Proceedings
(AIP Available online 1904)
卷期:
Volume 740,
issue 1
页码: 497-508
ISSN:0094-243X
年代: 1904
DOI:10.1063/1.1843530
出版商: AIP
数据来源: AIP
摘要:
Here we will present some spectroscopic methods for emission gas research in the emission line region of Active Galactic Nuclei (AGNs): (1) We will demonstrate the possibility to use the Boltzmann‐plot method to estimate the physical conditions in the broad line regions (BLRs); (2) We will discuss the applicability of so called “Gaussian method” for spectral line shape investigation of narrow line regions (NLRs) and BLRs; (3) We will present a method to fit the line profiles with a kinematically complex model. We apply a two‐component model assuming that the line wings originate in a very broad line region (VBLR) and the line core in an intermediate line region (ILR) of AGNs. The VBLR is assumed to be an accretion disk and the ILR a spherical emission region; (4) Also, a model for fitting of the broad absorption lines in quasars will be discussed. © 2004 American Institute of Physics
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