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Structure and Time-Dependent Behavior of Be Star Disks in Be/X-Ray Binaries

Published online by Cambridge University Press:  25 May 2016

A.T. Okazaki
A.T. Okazaki*
Affiliation:
College of General Education, Hokkai-Gakuen University, Toyohira-ku, Sapporo 062, Japan

Extract

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We consider the structure and time dependent behavior of the outflow in disks of Be stars in Be/X-ray binaries, based on the viscous decretion disk scenario (Lee et al. 1991). In this scenario, the matter ejected from the star with the Keplerian velocity at the equatorial surface of the star drifts outward because of the effects of viscosity, and forms the disk.

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. 362 - 363
Copyright
Copyright © Kluwer 1998 

References

Lee, U., Saio, H., Osaki, Y., 1991, MNRAS 250, 432 Google Scholar
Negueruela, I., Reig, P., Coe, M.J., Fabregat, J., 1997, submitted to A&A Google Scholar