Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....87l..15m&link_type=abstract
Astronomy and Astrophysics, vol. 87, no. 3, July 1980, p. L15-L17. Research supported by the United States-Israel Binational Sc
Astronomy and Astrophysics
Astrophysics
2
Stellar Mass Ejection, Stellar Models, Variable Stars, Asymmetry, Kinematics, Optical Thickness
Scientific paper
Deviations from the standard model of SS433 are considered. Mainly deviations in which the symmetry between the two line emitting regions is broken (such as a misalignment of the two velocity vectors) are considered. Even if the velocity vectors are constant in the rotating frame, the average wavelength of the two satellites is not constant with time but varies with the rotation period. Such as asymmetric system mimics a symmetric system with: (1) a periodically variable Lorentz factor (or velocity), (2) an average value of Lorentz factor or velocity which differs from the true value, and (3) periodically variable angle between the rotation axis and the velocity vectors.
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