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The spin-up of contracting red supergiants
ASTRONOMY & ASTROPHYSICS, no. 1 (1998): 210-220
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Abstract
We report on a mechanism which may lead to a spin-up of the surface of a rotating single star leaving the Hayashi line, which is much stronger than the spin-up expected from the mere contraction of the star. By analyzing rigidly rotating, convective stellar envelopes, we qualitatively work out the mechanism through which these envelopes m...More
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