Different velocity dependences of physical conditions of high- and low-ionization lines in broad-line regions

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作者
Snedden, SA [1 ]
Gaskell, CM [1 ]
机构
[1] New Mexico State Univ, Apache Point Observ, Sunspot, NM 88349 USA
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P1 [天文学];
学科分类号
0704 ;
摘要
We present results from a study of high- and low-ionization emission line ratios as a function of projected velocity for a sample of eight active galactic nuclei (AGNs). Our results are based on analysis of high signal-to-noise optical and Hubble Space Telescope (HST) UV spectra. Comparing the emission line ratios to those predicted by photoionization models indicates that the physical conditions responsible for the high-ionization emission lines axe consistent with a wind, whereas those of the low-ionization lines axe consistent with a virialized disk.
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页码:197 / 200
页数:4
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