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Preprint typeset using L ATEX style emulateapj v. 10/09/06 LARGE-SCALE MAGNETIC FIELDS IN STELLAR INTERIORS I – RELAXED EQUILIBRIUM CONFIGURATIONS TO MODEL FOSSIL FIELDS

By V. Duez and S. Mathis

Abstract

In this short paper, we thus revisit the pioneer work by Prendergast (1956) who derived such mixed poloidaltoroidal magnetic configurations by solving the magnetohydrostatic equilibrium of incompressible spheres (see also Chandrasekhar & Prendergast 1956). The obtained configurations seem to be relevant in regard of the most recent numerical simulations that may explain fossil fields in early-type stars, white dwarfs or neutron star

Year: 2009
OAI identifier: oai:CiteSeerX.psu:10.1.1.315.8234
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