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VRI Light Curve Analysis of SS 433
Published online by Cambridge University Press: 25 May 2016
Extract
In the light curves of SS 433, in addition to a binary modulation with a period of 13.1 d, there is a precessional one with a period of 162.5 d (Kemp et al. 1986). In the current studies, however, the attention was focused mainly on the light curves during eclipse (see, however, e.g., Antokhina, Cherepashchuk 1987). Thus, in this paper we examine light curves during precession and compare them with observational ones (Fukue et al. 1997b).
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- Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
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- Copyright © Kluwer 1998