Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.209..607m&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 209, Aug. 1, 1984, p. 607-639.
Astronomy and Astrophysics
Astronomy
29
Magnetic Stars, Stellar Magnetic Fields, Stellar Models, Stellar Rotation, Stellar Structure, Magnetic Field Configurations, Stellar Evolution
Scientific paper
The solutions obtained by the application of a novel numerical technique to the problem of the structure of axisymmetric rotating magnetic stars are found to differ from those of Mestel and Moss (1977), in that a time-dependent version of the MHD equation is solved on a two-dimensional grid. Models rotating relatively rapidly, which retain a comparatively low ratio of internal to surface magnetic flux over ohmic time-scales, can be found. It is suggested that the properties of rapidly rotating models with large angles chi between their axes may be radically different from those with small chi, inasmuch as magnetic flux concentration beneath the surface is not likely to occur for large chi.
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