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Mass loss from hot stars below the main sequence
Published online by Cambridge University Press: 12 April 2016
Abstract
The evolutionary implications of mass loss from post-asymptotic giant branch stars is discussed, with reference to the UV observations of sdO's.
- Type
- Session I - Winds from Early Type Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 71 - 74
- Copyright
- Copyright © Reidel 1981