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Variable Stellar Wind from the WN-Star HD 151932
Published online by Cambridge University Press: 12 April 2016
Abstract
The effects of the interaction of strong Wolf-Rayet stellar wind with the surrounding interstellar medium in ring-type nebulae are briefly discussed.
The outstanding variability of the envelope of the WN 7 star HD 151932 is explained by small density fluctuations. Variable WR wind may be the reason for the filamentary structure observed in ring-type nebulae.
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- Part III: Evolved Stars
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- Copyright © Veröff. Der Remeis-Sterwarte 1977