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The role of magnetic fields in governingthe angular momentum evolution ofsolar-type stars

Published online by Cambridge University Press:  03 November 2009

C. Neiner ,
J.-P. Zahn  and
J. Bouvier
J. Bouvier*
Affiliation:
Laboratoire d'Astrophysique, Observatoire de Grenoble, Université J. Fourier, CNRS, BP. 53, 38041 Grenoble Cedex 9, France
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Abstract

I review the development of ideas regarding the angular momentumevolution of solar-type stars, from the early 60's to the most recentyears. Magnetic fields are the central agent that dictates therotational evolution of solar-type stars, both during the pre-mainsequence, through star-disk magnetic coupling, and during the mainsequence, through magnetized winds. Key theoretical developments aswell as important observational results are summarized in this review.

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Type
Research Article
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European Astronomical Society Publications Series , Volume 39: Stellar Magnetism , 2009 , pp. 199 - 209
Copyright
© EAS, EDP Sciences, 2009

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