Mass-Radius Relation for Magnetic White Dwarfs

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© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation In-Saeng Suh and G. J. Mathews 2000 ApJ 530 949 DOI 10.1086/308403

0004-637X/530/2/949

Abstract

Recently, several white dwarfs with very strong surface magnetic fields have been observed. In this paper we explore the possibility that such stars could have sufficiently strong internal fields to alter their structure. We obtain a revised white dwarf mass-radius relation in the presence of strong internal magnetic fields. We first derive the equation of state for a fully degenerate ideal electron gas in a magnetic field using an Euler-MacLaurin expansion. We use this to obtain the mass-radius relation for magnetic 4He, 12C, and 56Fe white dwarfs of uniform composition.

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10.1086/308403