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Variable Stellar Wind from the WN-Star HD 151932
Published online by Cambridge University Press: 12 April 2016
Abstract
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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.
- Type
- Part III: Evolved Stars
- Information
- Copyright
- Copyright © Veröff. Der Remeis-Sterwarte 1977
References
Johnson, H.M.
1973, in Wolf-Rayet and High Temperature Stars p. 42, Eds. Bappu, M.K.V., Sahade, J., IAU Symp. No. 49Google Scholar
Pikel’ner, S.B., Shcheglov, P.V.
1969, Astron. Zh.
45, 953; Soviet Astron. A.J.
12:, 757
Google Scholar
Smith, L.F.
1973, in Wolf-Rayet and High Temperature Stars p. 139, Eds. Bappu, M.K.V., Sahade, J., IAU Symp. No. 49Google Scholar
Smith, L.F.
1974, Proc. Second European Regional Meeting Astron., Mem. Soc. Astron. Italiana, 45, 367
Google Scholar
Wendker, H.J., Smith, L.F., Israel, F.P., Habing, H.J., Dickel, H.R.
1975, Astron. & Astrophys.
42, 173
Google Scholar