A phenomenological triple star scenario for SS 433

Details A phenomenological triple star scenario for SS 433 A phenomenological triple star scenario for SS 433

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...305..333f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 305, June 1, 1986, p. 333-335.

Astronomy and Astrophysics

Astrophysics

12

Precession, Stellar Models, Stellar Motions, Triple Stars, X Ray Binaries, B Stars, Stellar Evolution, Stellar Orbits

Scientific paper

It is suggested that SS 433 is a triple star, containig a short-period (1.5 d) binary like Sco X-1, orbiting a massive OB star in 13 d. Polar jets produced by the Sco X-1-like close binary can precess, with the period observed, if this binary is misaligned with the larger binary. The possible evolutionary history of such a system is discussed, starting from a triple star somewhat like either Lambda Tau or VV Ori.

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