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Alfvén waves and radiation pressure in the winds of Wolf-Rayet stars
Published online by Cambridge University Press: 07 August 2017
Abstract
We recently showed that Alfvén waves acting jointly with radiation pressure in Wolf-Rayet winds can possibly solve the momentum problem (dos Santos, Jatenco-Pereira and Opher 1993a, 1993b). In these analyses, however, constant radiation luminosity as a function of the distance to the star was assumed. We impose here conservation of the energy flux and examine the effect on the radiation luminosity.
Keywords
- Type
- Session II - Model atmospheres for single Wolf-Rayet stars
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- Copyright © Kluwer 1995