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Radiative transfer in the broad emission line regions of quasi-stellar objects

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/166550· OSTI ID:6744049
The accuracy of the simplifying approximations usually made to avoid solving in detail the equations of radiative transfer from broad emission line regions of quasi-stellar objects is examined. Starting with a pure hydrogen model, the effects are considered of including heavy-element cooling, helium and X-ray opacity, X-ray heating, Lyman continuum transfer replacing on-the-spot approximation, and line transfer with Lyman-alpha partial redistribution replacing escape probabilities. The hydrogen statistical equilibrium equations are solved in detail. 40 references.
Research Organization:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
OSTI ID:
6744049
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 331; ISSN ASJOA
Country of Publication:
United States
Language:
English