A precise solution for the spectral line profile originating in a luminous ring around a black hole

Details A precise solution for the spectral line profile originating in a luminous ring around a black hole A precise solution for the spectral line profile originating in a luminous ring around a black hole

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20..508d&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 4, p. 508-508.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The light emitted by a luminous ring in Kepler motion around a black hole is subject to both Doppler and gravitational spectral shifts. In this paper a rigorous solution is obtained for a Lorentz profile under the Schwarzschild metric. Its relevance to the identification of spectral line of the quasar 1604+179 in the Hercules cluster of galaxies is discussed.

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