Periodicities in the photometric variability of SS 433

Details Periodicities in the photometric variability of SS 433 Periodicities in the photometric variability of SS 433

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..605c&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, July 1991, p. 605-612. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Accretion Disks, Eclipsing Binary Stars, Light Curve, Periodic Variations, Stellar Flares, Stellar Spectrophotometry, Cataclysmic Variables, Fourier Analysis, Relativistic Effects

Scientific paper

Periodicities in the light variations of SS 433 are analyzed on the basis of observations made between 1978 and 1988. The nature of regular photometric variability with periods of 162.5, 13.092, and 6.296 d is investigated and the flare activity of SS 433 is analyzed. A quasi-period of about 26 d in the variability of the shape of the primary minimum of the light curve is found.

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