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Discrete Components in OB and Be Stars: The Shocking Truth?
Published online by Cambridge University Press: 23 September 2016
Abstract
Preliminary calculations of the absorption profiles produced if multiple shells are ejected from the photosphere into a non-monotonic wind, suggest that this geometrical model can reproduce a wide variety of simple and complex profiles observed in the discrete components in OB and Be stars.
- Type
- IV. Models
- Information
- International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 431 - 433
- Copyright
- Copyright © Cambridge University Press 1987