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Observational aspects of Wolf-Rayet atmospheres

Published online by Cambridge University Press:  07 August 2017

I. I. Antokhin*
Affiliation:
Sternberg State Astronomical Institute Universitetskij pr., 13, Moscow 119899, Russia

Abstract

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Observational data suggest that WR atmospheres must be considered as highly inhomogeneous objects incorporating strong shocks induced by radiative instability and full-scale supersonic turbulence, with relatively small mean mass-loss rates.

Type
Session II - Model atmospheres for single Wolf-Rayet stars
Copyright
Copyright © Kluwer 1995 

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