On the effective magnetic field of an oblique rotating star with an axisymmetric magnetic field

Details On the effective magnetic field of an oblique rotating star with an axisymmetric magnetic field On the effective magnetic field of an oblique rotating star with an axisymmetric magnetic field

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....95..240g&link_type=abstract

Astronomy and Astrophysics, vol. 95, no. 2, Mar. 1981, p. 240-243.

Astronomy and Astrophysics

Astrophysics

1

A Stars, Magnetic Stars, Stellar Magnetic Fields, Stellar Rotation, Magnetic Field Configurations, Poloidal Flux, Stellar Models, Surface Geometry, Symmetry

Scientific paper

This study considers first the theoretical determination of the effective magnetic field in an oblique rotating and magnetic star. An analytical expression for the variation of the effective field is derived for a surface distribution of a magnetic field that is axisymmetric about an axis through the stellar centre, but that is not necessarily irrotational. Subsequently, it is shown that the effective-field observations only contain partial information on the surface distribution of a magnetic field if it is assumed to be axisymmetric but not irrotational.

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