http://arxiv.org/abs/1811.04416
The purpose of this short paper is to give a summary of the derivation of a perturbative method to assess the impact of an arbitrary 3D magnetic field configuration, whose energy is everywhere small relative to the gravitational binding energy, on the form and value of the eigenfrequencies and eigenfunctions of stellar oscillations.
K. Augustson and S. Mathis
Tue, 13 Nov 18
16/74
Comments: 4 pages; Proceedings of the 2018 meeting of the Soci\’et\’e Fran\c{c}aise d’Astronomie et d’Astrophysique
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