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Mixing in Magnetized Interiors of Solar-Type Stars: Frequently Asked Questions

Published online by Cambridge University Press:  30 March 2016

Paul Charbonneau
Paul Charbonneau*
Affiliation:
HAO/NCAR, P.O. Box 3000, Boulder, CO 80307, U.S.A.

Abstract

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This short paper discusses various issues pertaining to the redistribution of angular momentum and mixing of chemical species in the radiative interior of solar-type stars. Results obtained to date indicate that models combining magnetically-mediated angular momentum transport with turbulent mixing of chemical species offer the best hope of explaining the observed rotation and light element evolution in open clusters, without doing excess violence to seismic measurements of the solar internal differential rotation.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 301 - 303
Copyright
Copyright © Astronomical Society of Pacific 2002

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