Magnetohydrodynamical winds with finite electrical conductivities.

Physics

Scientific paper

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Scientific paper

The authors discuss a numerical treatment of the resistive MHD winds which are driven by strongly magnetized, rotating stars. For simplicity, the axis of rotation is assumed to coincide with that of magnetization. It is shown that rotation-driven wind solutions surely exist, to the set of resistive MHD equations even when the stellar magnetic fields remain of closed type.

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