Time-dependent models of magnetic stars. IV - Perpendicular axes

Details Time-dependent models of magnetic stars. IV - Perpendicular axes Time-dependent models of magnetic stars. IV - Perpendicular axes

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.226..281m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 226, May 15, 1987, p. 281-296.

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Axes Of Rotation, Magnetic Stars, Main Sequence Stars, Stellar Magnetic Fields, Stellar Models, Stellar Rotation, Computational Astrophysics, Magnetic Field Configurations, Self Consistent Fields, Stellar Evolution, Time Dependence

Scientific paper

The evolution of large-scale initially axisymmetric fields immersed in middle main-sequence stellar models is followed in the case where the rotation axis and initial field axis are strictly perpendicular. The prediction that in this case the surface flux is never buried by the modified Eddington-Sweet circulation is verified, although mode-mixing may eventually reduce the strength of the dipolar field component. It appears that non-axisymmetric field components will grow over time-scales of 108yr or so. Effects of differing initial field geometries are discussed.

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