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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
Extract
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.
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- Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
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- Copyright © Kluwer 1998