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On the possibility of partial matter mixing in rotating massive stars

Published online by Cambridge University Press:  26 May 2016

Eugenij I. Staritsin
Eugenij I. Staritsin*
Affiliation:
Astronomical observatory, Ural State University, pr. Lenina 51, Yekaterinburg, 620083 Russia

Abstract

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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.

Type
Part 2. Interiors of Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 427 - 428
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Lang, K.R. 1974, Astrophysical Formulae, Vol. 1 (Berlin: Springer), ch.3.Google Scholar
Maeder, A. 1997, A&A 321, 134.Google Scholar
Staritsin, E.I. 2001, Astron. Reports 45, 467.Google Scholar
Talon, S., Zahn, J.-P. 1997, A&A 317, 749.Google Scholar