Modelling magnetic oscillators

Details Modelling magnetic oscillators Modelling magnetic oscillators

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.118a2018s&link_type=abstract

Journal of Physics: Conference Series, Volume 118, Issue 1, pp. 012018 (2008).

Physics

2

Scientific paper

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.

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