Stellar dynamos - theoretical aspects

Details Stellar dynamos - theoretical aspects Stellar dynamos - theoretical aspects

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005an....326..254d&link_type=abstract

Astronomische Nachrichten, Vol.326, Issue 3, p.254-264

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4

Binaries: Close, Stars: Late-Type, Stars: Magnetic Fields, Stars: Pre-Main Sequence

Scientific paper

I review some dynamo models and constraints for stars other than the Sun. The models include mean-field dynamo models for RS Cvn binary systems and global magnetoconvection simulations for supergiants and for fully convective stars. In the latter case, we find generation of mixed-parity large-scale magnetic fields once the dynamo reaches saturation. In addition to the cool, narrow downdrafts known from local simulations, these models also show a hot convective plume stretching from the centre towards the surface.

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