Precession instability models of SS433

Details Precession instability models of SS433 Precession instability models of SS433

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.202..113l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 202, no. 1, p. 113-120.

Statistics

Computation

Astronomical Models, Regression Analysis, X Ray Binaries, Computational Astrophysics, Error Analysis, Numerical Stability

Scientific paper

Sinusoidal and damped sinusoidal models are analyzed and compared in terms of phase residual. An improved damped sinusoidal model is proposed. The data from the three models are subjected to regression analysis in order to determine their differences. It is concluded that the improved damped sinusoidal model describes the phase residual distribution of the jet precession of SS433 better than the other models.

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