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

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acaps..11..321c&link_type=abstract

(Acta Astrophysica Sinica, vol. 11, no. 4, 1991, p. 321-326) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 1

Statistics

Computation

Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Computational Astrophysics, Line Shape, Line Spectra, Doppler Effect, Emission Spectra, Molecular Clouds, Red Shift, Schwarzschild Metric

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. All these effects were taken 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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