Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1971
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..14..464r&link_type=abstract
Astrophysics and Space Science, Volume 14, Issue 2, pp.464-472
Astronomy and Astrophysics
Astrophysics
22
Scientific paper
The possible existence of strong magnetic fields in stars is discussed and a method of constructing highly distorted models of magnetic, rotating stars developed. For stars with both poloidal and toroidal fields at the surface a force-free outer boundary condition is necessary. Non-linear solutions of the force-free equations must be used. The force-free equations and the structure equations for a white dwarf are solved simultaneously by a finite difference method.
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