Line profiles of the two-phase medium broad-line region in active galactic nuclei.

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Active Galactic Nuclei: Broad-Line Regions, Active Galactic Nuclei: Line Profiles

Scientific paper

In the framework of BLR in AGNs a delicate radiation model for a typical emission cloud is established, in which the backside photoionization of the cloud against the central continuum source by the scattered diffuse continuum in the hot medium is considered. Under the assumption of the radial kinematics of the BLR clouds, the line profiles for the two important UV emission-lines, Lyα and C IV λ1549 are computed. Based on these calculations, various physical factors that affect the properties of the emission-line profiles are discussed.

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