Line profiles of radially moving clouds in the presence of an accretion disk

Details Line profiles of radially moving clouds in the presence of an accretion disk Line profiles of radially moving clouds in the presence of an accretion disk

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cha%26a..16...17c&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 16, Issue 1, p. 17-23.

Astronomy and Astrophysics

Astrophysics

1

Active Galactic Nuclei-Radially Moving Clouds -Accretion Disk

Scientific paper

In the black hole model of active galactic nuclei, light rays emitted by ionized clouds moving in the vicinity of the black hole will be subjected to the effects of doppler shift, gravitational redshift and bending, as well as shielding by accretion disk, should this exist. We have taken all these effects into consideration in a rigorous solution of the photon transport equation for the line profile under the Schwarzschild metric. It is found that asymmetric double peak structure appears in some cases.

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