Profiles of spectral lines of an accretion ring around a Kerr black hole

Details Profiles of spectral lines of an accretion ring around a Kerr black hole Profiles of spectral lines of an accretion ring around a Kerr black hole

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.113..181z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 113, no. 1, July 1985, p. 181-187.

Astronomy and Astrophysics

Astronomy

1

Accretion Disks, Black Holes (Astronomy), Line Spectra, Ring Structures, Stellar Mass Accretion, Deflection, Distribution Functions, Doppler Effect, Kinetic Equations, Photons, Red Shift

Scientific paper

Profiles of spectral lines emitted from an accretion ring around an object with strong gravitational field should be affected by Doppler shift, gravitational redshift, and deflection of light. Taking these effects into account, precise line profile of a Keplerian ring around a Kerr black hole for a distant observer is obtained by solving the kinetic equation of photons.

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