Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.158...27z&link_type=abstract
"Communications in Asteroseismology, Vol.158, p. 27 Proceedings of "38th Liege International Astrophysical Colloquium: Evolutio
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
Magnetic fields responsible for various activity phenomena have been detected at the surface of many stars. Presumably they are also present in the stars' deep interior. They channel stellar winds to large distance, thus increasing the loss of angular momentum. In stably stratified radiation zones, they tend to impose uniform rotation, and may thus interfere with the rotational mixing operating in these regions and influence the evolution of the host star. Moreover, certain magnetic configurations are known to be unstable, and they could produce some mixing of their own. We shall discuss these problems in the light of the latest developments.
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