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Mass loss from hot stars below the main sequence

Published online by Cambridge University Press:  12 April 2016

R. Viotti ,
L. Rossi  and
F. D'Antona
R. Viotti
Affiliation:
Istituto Astrofisica Spaziale, CNR, Frascati, Italy
L. Rossi
Affiliation:
Istituto Astrofisica Spaziale, CNR, Frascati, Italy
F. D'Antona
Affiliation:
Osservatorio Astronomico, Roma, Italy

Abstract

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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

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