Cyclical Variability in Stellar Winds pp 344-344 | Cite as
Variabilities in Be-Star Disks in Be/X-Ray Binaries
Conference paper
Abstract
We examine long-term, cyclic variabilities of the outflow in the disks of Be stars in Be/X-ray binaries in the context of the viscous decretion disk scenario. In this scenario, the matter ejected from the equatorial surface of the star with the Keplerian rotation velocity drifts outward because of viscosity and forms a disk (Lee et al. 1991).
References
- Lee, U., Saio, H., Osaki, Y. (1991): MNRAS 250, 432ADSGoogle Scholar
- Negueruela, I., Reig, P., Coe, M.J., Fabregat, J. (1998): A A, in pressGoogle Scholar
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© Springer-Verlag Berlin Heidelberg 1998