A kinematic model for SS433

Details A kinematic model for SS433 A kinematic model for SS433

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.279..701a&link_type=abstract

Nature, vol. 279, June 21, 1979, p. 701-703. NSF-supported research.

Astronomy and Astrophysics

Astronomy

160

Emission Spectra, Periodic Variations, Radio Sources (Astronomy), Red Shift, Doppler Effect, Helium, Hydrogen, Radial Velocity

Scientific paper

A kinematic model for the bizarre emission-line object SS433 is proposed in which the radiation with variable Doppler shift is emitted by hot matter ejected from the central object at high but nearly constant velocity in oppositely directed narrow streams, possibly along a magnetic axis. According to this model, rotation of the beam axis provides the observed radial-velocity variations, and the observed emission is produced when matter reaches a critical distance from the central object and cools sufficiently to recombine. Specific predictions are made regarding the behavior of the variable velocity components during the as-yet unobserved portions of the 164-day period.

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