A non-axisymmetric rigid rotator model for magnetic stars

Details A non-axisymmetric rigid rotator model for magnetic stars A non-axisymmetric rigid rotator model for magnetic stars

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.172..133s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 172, July 1975, p. 133-139.

Astronomy and Astrophysics

Astronomy

52

Astronomical Models, Dynamo Theory, Magnetic Stars, Magnetic Variations, Stellar Rotation, Magnetic Dipoles, Magnetic Field Configurations, Phase Shift

Scientific paper

A generalized, nonaxisymmetric decentred dipole model is proposed to explain asymmetric magnetic variations and phase shifts between the respective extrema of effective field and surface field of magnetic stars. Detailed models are derived for two stars and it is shown that the model can reproduce the observed magnetic variations of all well-known magnetic stars but one.

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