The effect of toroidal magnetic field and differential rotation on self-gravitating polytropic models. II

Details The effect of toroidal magnetic field and differential rotation on self-gravitating polytropic models. II The effect of toroidal magnetic field and differential rotation on self-gravitating polytropic models. II

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.201..229g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 201, no. 2, p. 229-241.

Statistics

Computation

4

Astronomical Models, Magnetic Field Configurations, Polytropic Processes, Rotating Bodies, Computational Astrophysics, Gravitational Effects, Perturbation Theory

Scientific paper

In this paper we compute differentially rotating polytropic models distorted by toroidal magnetic field. In particular, we study rotating sequences, which do not terminate with a critical rotation. In the computations we use the so-called 'complex-plane strategy' and 'multiple partition technique', which are numerical methods developed recently by the first author.

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