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Magnetic-Loop Model For Be Stars (Review Paper)
Published online by Cambridge University Press: 23 September 2016
Abstract
The magnetic-loop model for a stellar mantle is described and it is shown how this model may be used to understand the differences in spectrum and change of spectrum which are observed for main-sequence stars haying effective.temperatures in the range from 2.5 x 104 to 3.0 x 104 K.
It is suggested that the difference in spectrum between a shell star such as Gamma Cas when it is in an active state and a Wolf-Rayet star may be due to a difference in environment.
- Type
- IV. Models
- Information
- International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 411 - 427
- Copyright
- Copyright © Cambridge University Press 1987
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