The Model of the Peculiar Object SS433

Details The Model of the Peculiar Object SS433 The Model of the Peculiar Object SS433

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58....3b&link_type=abstract

Astronomicheskii Zhurnal, Vol. 58, P. 3, 1981

Astronomy and Astrophysics

Astronomy

3

Scientific paper

A model is devised for the object SS 433 to fit the observed radial-velocity curve of the moving emission lines better than does Abell and Margon's kinematic model. SS 433 is taken to be a close binary system of orbital period P2 = 13d, comprising an optical star and a neutron star surrounded by a gaseous accretion disk precessing with a period P1 = 164d. The magnetic dipole axis of the rapidly spinning neutron star is normal to the rotation axis. Relativistic particles stream out of the megnetic poles and strip a pair of gas jets from the accretion disk. The physical processes that should operate in such a system are discussed and several predictions of observable phenomena are made

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