A model for radio and X-ray emission from SS433

Details A model for radio and X-ray emission from SS433 A model for radio and X-ray emission from SS433

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.276.1191r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 276, Issue 4, pp. 1191-1196.

Physics

6

Accretion, Accretion Discs, Black Hole Physics, Plasmas, Radio Continuum: Stars, X-Rays: Stars

Scientific paper

Super-Eddington accretion on to a stellar mass black hole is the most plausible model for the well-known object SS433. We discuss some relevant physical properties of accretion discs around stellar mass black holes and present a model for the radio spectrum and X-ray emission from SS433 that is constrained by inferred jet mass-loss rates and luminosity as well as radio flux density and X-ray measurements. We discuss electron acceleration in the bipolar jets for both quasi-stationary and impulsive scenarios for mass ejection and conclude that the magnetic field in the radio- and X-ray-emitting regions of the jets probably originated in the accretion disc, where it supplies the required viscosity.

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