Modelling magnetic oscillators

Hideyuki Saio

Research output: Contribution to journalArticle

5 Citations (Scopus)

Abstract

The effect of magnetic fields complicates the analysis of nonradial pulsations of stars. The angular dependence of the eigenfunction of a pulsation mode cannot be represented by a single spherical harmonic, and another type of oscillations enters into the equations. We discuss different methods employed to analyse nonradial pulsations in the presence of a magnetic field and compare the results from the different methods. Then, we discuss some important properties caused by the presence of a strong magnetic field, and discuss some asteroseismological works.

Original languageEnglish
Article number012018
JournalJournal of Physics: Conference Series
Volume118
Issue number1
DOIs
Publication statusPublished - 2008 Jul 1
Externally publishedYes

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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