Precise solution of line profiles for a black hole with a luminous ring in its accretion disk.

Details Precise solution of line profiles for a black hole with a luminous ring in its accretion disk. Precise solution of line profiles for a black hole with a luminous ring in its accretion disk.

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..227d&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 3, p. 227 - 230

Astronomy and Astrophysics

Astrophysics

1

Black Holes: Accretion Disks, Quasars: Emission Spectra

Scientific paper

The light, originally in Lorentz spectral type, emitted from a luminous Keplerian ring around a black hole should be affected by Doppler shift and gravitational redshift and deflection. A double-peaked line profile should be received by a faraway observer. The precise solution of line profile is obtained in the Schwarzschild case in this paper. The emission spectrum identification of the quasar 1604+179 in the Hercules Cluster is also discussed according to the relative intensity of the two peaks in the double-peaked profile.

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