Physical characteristics of critically distorted or almost spherically shaped rotating magnetic polytropic models |
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Authors: | PJ Papasotiriou VS Geroyannis |
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Institution: | (1) Astronomy Laboratory, Department of Physics, University of Patras, Greece |
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Abstract: | We use the so-called complex plane iterative technique (CIT) to the computation of polytropic stars distorted by rotation
(either rigid or differential) and magnetic fields (both toroidal and poloidal). We give emphasis on computing(i) critically
rotating configurations, and (ii) configurations that – dueto the counterbalancing of the effects of rotation and poloidal
magnetic field with the effects of toroidal magnetic field – obtain an almost spherical shape.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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