Rotating Visco-Polytropic Models: Dissipative Effects under the Influence of a Toroidal Magnetic Field

Details Rotating Visco-Polytropic Models: Dissipative Effects under the Influence of a Toroidal Magnetic Field Rotating Visco-Polytropic Models: Dissipative Effects under the Influence of a Toroidal Magnetic Field

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.232..149g&link_type=abstract

Astrophysics and Space Science, Volume 232, Issue 1, pp.149-166

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

In this paper we consider dissipative effects by viscous friction of differentially rotating visco-polytropic models that are further distorted by a toroidal magnetic field. In particular, we study numerically rotating visco-magnetopolytropes by implementing the so-called “complex-plane iterative technique” (CIT), developed by the first author and used in the recent past for computing rotating models of polytropes and white dwarfs. We emphasize on dissipative effects and discuss some interesting scenarios concerning coupling of a magnetic star with its environment.

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