SS 433 as a black hole candidate

Details SS 433 as a black hole candidate SS 433 as a black hole candidate

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11...10a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Jan. 1985, p. 10-16) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Jan.-Feb.

Astronomy and Astrophysics

Astronomy

5

Accretion Disks, Astronomical Models, Black Holes (Astronomy), Light Curve, Luminescence, Photometry, Stellar Radiation

Scientific paper

The inverse optical light curves of SS 433 are interpreted within the framework of a geometrically thick model of an accretion disk surrounding a compact relativistic object. Conditions are established for the relativistic object to be a black hole. Computer-plot drawings show the precessing, geometrically thick accretion disk undergoing eclipse by a normal OB star.

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