SS433 - Another view

Details SS433 - Another view SS433 - Another view

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986comap..11..201k&link_type=abstract

Comments on Modern Physics, Part C - Comments on Astrophysics (ISSN 0146-2970), vol. 11, Sept. 1986, p. 201-211.

Astronomy and Astrophysics

Astrophysics

20

Accretion Disks, Astronomical Models, Binary Stars, Plasma Jets, Stellar Models, X Ray Sources, Companion Stars, Emission Spectra, Line Spectra, Stellar Mass Accretion, Stellar Mass Ejection

Scientific paper

Theoretical models of SS433 are reviewed, with special attention to accretion-disk dynamics and the 6-d periodicity, line locking, the efflux rate, and analogies between SS433 and other objects. Models in which the motion of the oppositely directed jets is explained by the precession of the entire accretion disk under the influence of a binary companion (e.g., Katz, 1980; van den Heuvel et al., 1980) are found to be most attractive, although they do not adequately explain all of the observed phenomena. It is considered more justifiable to compare SS433 with bipolar nebulae than with extragalactic jets, since the latter appear to be nonthermal phenomena.

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