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Peculiar Intrinsic Parameters of Massive Stars as a Result of an Early Phase of Homogeneous Evolution
Published online by Cambridge University Press: 12 April 2016
Abstract
Rotationallly induced mixing can explain several observational peculiarities of massive stars. Homogeneous evolution of differentially rotating stars including spindown due to stellar winds is studied by means of homology transformations of ZAMS models.
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- V. The changing interior
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- Copyright © Astronomical Society of the Pacific 1993
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