The splitting of non-radial modes of oscillation in rotating magnetic stars

Details The splitting of non-radial modes of oscillation in rotating magnetic stars The splitting of non-radial modes of oscillation in rotating magnetic stars

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..135m&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 1-2, May 1980, p. 135-137.

Astronomy and Astrophysics

Astrophysics

3

Magnetic Stars, Oscillations, Stellar Models, Stellar Rotation, Vibration Mode, Splitting, Stellar Magnetic Fields

Scientific paper

The splitting of adiabatic non-radial modes of oscillation in self-consistent models of uniformly rotating magnetic stars is investigated. It is found that, for reasonable values of the stellar parameters, the joint (second order) magnetic and rotational splitting may be large enough to be observable in massive main sequence stars, and for some p modes it may be comparable with the first order rotational splitting.

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