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Stellar models of rotating, pre-main sequence low-mass stars with magnetic fields

Published online by Cambridge University Press:  07 August 2014

Luiz T. S. Mendes ,
Natália R. Landin  and
Luiz P. R. Vaz
Luiz T. S. Mendes
Affiliation:
Depto. de Engenharia Eletrônica, UFMG, 31270-901 Belo Horizonte, MG, Brazil email: luizt@cpdee.ufmg.br Depto. de Física, UFMG, 31270-901 Belo Horizonte, MG, Brazil email: vaz@fisica.ufmg.br
Natália R. Landin
Affiliation:
UFV, Campus Florestal, 35690-000 Florestal, MG, Brazil email: nlandin@ufv.br Depto. de Física, UFMG, 31270-901 Belo Horizonte, MG, Brazil email: vaz@fisica.ufmg.br
Luiz P. R. Vaz
Affiliation:
Depto. de Física, UFMG, 31270-901 Belo Horizonte, MG, Brazil email: vaz@fisica.ufmg.br
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Abstract

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We report our present efforts for introducing magnetic fields in the ATON stellar evolution code code, which now evolved to truly modifying the stellar structure equations so that they can incorporate the effects of an imposed, large-scale magnetic field. Preliminary results of such an approach, as applied to low-mass stellar models, are presented and discussed.

Keywords

Stars: Magnetic fieldsStars: EvolutionStars: Rotation

References

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