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Modeling mass loss from B[e] stars
Published online by Cambridge University Press: 12 April 2016
Extract
It has been suggested by Zickgraf et al. (1986) that the outer atmosphere of some B[e] stars has a two-component structure: a fast, radiation-driven wind from the pole, and a dense, slow outflow from the equator. This is also die basic picture investigated by Poe, Friend, and Cassinelli (1989) (hereafter PFC) to explain the momentum problem associated with Wolf-Rayet stars. Here we apply the PFC multiforce wind theory to model the B[e] outflow phenomenon.
- Type
- Section I: Main Papers, General Discussions, and Two Panel Discussions
- Information
- International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 121 - 126
- Copyright
- Copyright © Kluwer 1989