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VRI Light Curve Analysis of SS 433

Published online by Cambridge University Press:  25 May 2016

Masamitsu Okugami ,
Yoshimi Obana  and
Jun Fukue
Masamitsu Okugami
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582, Japan
Yoshimi Obana
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582, Japan
Jun Fukue
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582, Japan

Extract

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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).

Type
Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 364 - 365
Copyright
Copyright © Kluwer 1998 

References

Antokhina, É.A., Cherepashchuk, A.M. 1987, SvA 31, 295 Google Scholar
Fukue, J. et al. 1997a, PASJ 49, 93 Google Scholar
Fukue, J. et al. 1997b, submitted to PASJ Google Scholar
Kemp, J.C. et al. 1986, ApJ 305, 805 Google Scholar
Tajima, Y., Fukue, J. 1996, PASJ 48, 529 Google Scholar