Angular momentum transport in pre-main-s
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C. Vigneron; A. Mangeney; C. Catala; E. Schatzman
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Article
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1990
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Springer
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English
โ 658 KB
Pre-Main-Sequence stars with masses between 2 and 5 M e (Herbig Ae/Be stars) have radiative subphotospheric envelopes. However, they possess strong stellar winds and show definite signs of activity which could be linked to surface magnetic field. Therefore, they must lose angular momentum at a signi