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On the possibility of partial matter mixing in rotating massive stars
Published online by Cambridge University Press: 26 May 2016
Abstract
The principal role of strong horizontal diffusion in overcoming the inhibiting effect of mean molecular weight gradient and in producing partial matter mixing between convective core and radiative envelope of a rotating star, is shown.
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- Part 2. Interiors of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003