SS433 - A black hole candidate?

Details SS433 - A black hole candidate? SS433 - A black hole candidate?

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..581z&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Feb. 1, 1989, p. 581-588.

Astronomy and Astrophysics

Astronomy

16

Black Holes (Astronomy), Eclipsing Binary Stars, Stellar Mass Accretion, Stellar Models, Celestial Mechanics, Neutron Stars, Stellar Mass, X Ray Sources

Scientific paper

The limits on the masses and dimensions of the components of the SS433 binary system derived by Stewart et al. (1987) are improved using an improved Roche lobe geometry. The new limits account for the fact that the accretion disk in the system may occupy a considerable fraction of the Roche lobe component. Using X-ray and optical observations, it is found that the mass of the object is about 10 solar masses, while the length of the X-ray jet is about 1.4 X 10 to the 12th cm.

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