On some possible additional relativistic effect in SS433

Details On some possible additional relativistic effect in SS433 On some possible additional relativistic effect in SS433

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...103l...7r&link_type=abstract

Astronomy and Astrophysics, vol. 103, no. 1, Nov. 1981, p. L7-L9.

Astronomy and Astrophysics

Astronomy

1

Angular Momentum, Black Holes (Astronomy), Eclipsing Binary Stars, Relativistic Effects, Stellar Mass Accretion, Stellar Models, Gravitational Fields, Red Shift, Stellar Rotation, Supernova Remnants

Scientific paper

In order to test the validity of the Lense-Thirring approximation (1918) in the context of models proposed for SS 433, a second-order theory of precession is developed. It is shown that if the matter is accreting into the black hole, the spin of the black hole is expected to change and, in turn, the observed precession period of 163.8 days due to the Lense-Thirring effect is going to change. The propagation of light signals within a few Schwarzschild radii of the black hole surface, in the ring models, may lead to the observation of further relativistic effects.

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