Acceleration, radiation and precession in SS 433

Details Acceleration, radiation and precession in SS 433 Acceleration, radiation and precession in SS 433

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236l.127k&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 236, Mar. 15, 1980, p. L127-L130.

Astronomy and Astrophysics

Astronomy

80

Plasma Acceleration, Precession, Radio Sources (Astronomy), Stellar Models, Stellar Winds, Supernova Remnants, Variable Stars, Emission Spectra, Frequency Shift, Gas Streams, Stellar Mass, Stellar Mass Accretion, X Ray Sources

Scientific paper

Some theoretical problems posed by the observations of SS 433 are considered. The monoenergetic beams point toward a gas-dynamic acceleration process. In this model the collimation implies that the acceleration occurs in a region of slab symmetry, possibly the surface layers of an accretion disk. The 164 day rotation of the beam pattern may be explained as a precession period.

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