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Is There Mass Loss in B Canis Majoris Stars?
Published online by Cambridge University Press: 12 April 2016
Extract
The purpose of this communication is to show that one possible explanation for the asymmetric line profiles observed in β Canis Majoris stars may be the presence of a stellar wind superimposed on a radial or nonradial pulsation.
- Type
- Part III: Evolved Stars
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- Copyright
- Copyright © Veröff. Der Remeis-Sterwarte 1977