Periods and Other Physical Parameters of Critically Distorted, or Almost Spherically Shaped, Rotating Magnetic White Dwarfs

Astronomy and Astrophysics – Astronomy

Scientific paper

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Magnetohydrodynamics: Mhd, Stars: Magnetic Fields, Stars: Rotation, Stars: White Dwarfs

Scientific paper

In this investigation we extend the so-called complex plane iterative technique (CIT) to the computation of classical white dwarf models distorted by rotation (either rigid or differential) and magnetic fields (both toroidal and poloidal). We give emphasis on computing (1) critically rotating configurations, and (2) almost spherical configurations due to counterbalancing of the effects of rotation and poloidal magnetic field with the effects of toroidal magnetic field.

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