A&A 411, 543-552 (2003)
DOI: 10.1051/0004-6361:20031491
Stellar evolution with rotation and magnetic fields
I. The relative importance of rotational and magnetic effects
A. Maeder and G. MeynetGeneva Observatory 1290 Sauverny, Switzerland
e-mail: Andre.Maeder@obs.unige.ch;georges.meynet@obs.unige.ch
(Received 28 May 2003 / Accepted 15 September 2003)
Abstract
We compare the current effects of rotation in stellar evolution to those of
the magnetic field created by the Tayler instability. In stellar
regions, where a magnetic field can be generated by the dynamo due to differential
rotation (Spruit 2002), we find that the growth rate
of the magnetic instability is much faster
than for the thermal instability. Thus, meridional circulation is small
with
respect to the magnetic fields, both for the transport of
angular momentum and of chemical elements. Also, the horizontal coupling by
the magnetic field, which reaches values of a few
105 G, is much more important than the effects
of the horizontal turbulence. The field, however, is not sufficient to distort the shape
of the equipotentials. We impose the condition that the energy of the magnetic field
created by the Tayler-Spruit
dynamo cannot be larger than the energy excess present in the differential
rotation. This leads to a criterion for the existence of the magnetic field
in stellar interiors.
Key words: stars: rotation -- stars: magnetic field -- stars: evolution
Offprint request: A. Maeder, Andre.Maeder@obs.unige.ch
© ESO 2003

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