The changing precession in SS433 - A critical study

Details The changing precession in SS433 - A critical study The changing precession in SS433 - A critical study

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984comap..10...53s&link_type=abstract

Comments on Modern Physics, Part C - Comments on Astrophysics (ISSN 0146-2970), vol. 10, Feb. 1984, p. 53-63. Research supported

Astronomy and Astrophysics

Astrophysics

8

Eclipsing Binary Stars, Precession, Stellar Mass Accretion, Stellar Models, Variable Stars, Accretion Disks, Collimation, Neutron Stars, O Stars, Stellar Luminosity

Scientific paper

It is now established that the 163 day precession period in SS433 is not constant but shortens and lengthens in a way which might be periodic. In addition, there is regular variation on a timescale of about 6 days, and faster irregular fluctuation. The authors discuss the disc models which have been proposed for this system and how they account for these effects. At the moment no model seems able to explain satisfactorily this interesting object.

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