Plasma Properties of the Broad Line Emitting Region in Active Galactic Nuclei

被引：0

作者：

Ilic, D. ^{[1
]}

Popovic, L. C. ^{[2
]}

Ciroi, S. ^{[3
]}

La Mura, G. ^{[3
]}

Rafanelli, P. ^{[3
]}

机构：

[1] Univ Belgrade, Fac Math, Dept Astron, Studentski Trg 16, Belgade 11000, Serbia

[2] Astron Observ, 11160 Belgrade, Serbia

[3] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy

来源：

SPACE PLASMA PHYSICS | 2009年 / 1121卷

关键词：

galaxies: active; quasars: emission lines; line: formation; plasmas; PHYSICAL-PROPERTIES; BALMER LINES; NGC; 5548; DIAGNOSTICS; MODELS; BLR;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In order to probe the physical properties of the emitting plasma in the broad line region (BLR) of active galactic nuclei (AGN), we perform a number of numerical simulations with the photoionization code CLOUDY. We investigate the Balmer and helium line ratios in order to find conditions in the BLR where so-called Boltzmann-plot (BP) method is applicable. We found correlations between average temperature, hydrogen density and He II/He I line ratio in the case where BP is present.

引用

页码：78 / +

页数：2

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