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Observational aspects of Wolf-Rayet atmospheres
Published online by Cambridge University Press: 07 August 2017
Abstract
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
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- Copyright © Kluwer 1995