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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
Abstract
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 112 - 113
- Copyright
- Copyright © International Astronomical Union 2014
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