Polytropic stellar models with a core-dynamo magnetic field

Details Polytropic stellar models with a core-dynamo magnetic field Polytropic stellar models with a core-dynamo magnetic field

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199..321m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 199, Apr. 1982, p. 321-330.

Astronomy and Astrophysics

Astronomy

5

Dynamo Theory, Magnetic Stars, Main Sequence Stars, Polytropic Processes, Stellar Magnetic Fields, Stellar Models, A Stars, Magnetic Field Configurations, Magnetohydrodynamics, Self Consistent Fields, Stellar Envelopes

Scientific paper

Self-consistent n = 3 polytropic models with a steady alpha-effect
dynamo operating in the inner 20 percent by radius are constructed.
These axisymmetric models are a first step towards developing
self-consistent models of upper main sequence stars with a dynamo field
generated in the convective core and pervading the radiative envelope.

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