A dissipative infall model for SS 433

Details A dissipative infall model for SS 433 A dissipative infall model for SS 433

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.191..411b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 191, May 1980, p. 411-415.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Earth Magnetosphere, Gravitational Collapse, H Alpha Line, Shock Wave Interaction, X Ray Sources, Doppler Effect, Energy Dissipation, Frequency Shift, Mass Flow Rate, Polarization Characteristics, Red Shift

Scientific paper

The data on SS 433 are analysed and found compatible with a model in
which the emission originates in shocks in matter falling through the
magnetosphere of a collapsed massive object. An observational test of
the model based on wing polarization of the shifted lines is proposed.

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