The Broad Line Regions of NGC 4151

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We compute the line strengths and profiles from a model of the cloud dynamics of the broad and intermediate line regions and compare the results with the observations of the Seyfert galaxy NGC 4151 in its various luminosity states.
30 pages

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/10367

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9602074
 http://arxiv.org/abs/astro-ph/9602074

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arXiv