The splitting of non-radial modes of oscillation in rotating magnetic stars
Abstract
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.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- May 1980
- Bibcode:
- 1980A&A....85..135M
- Keywords:
-
- Magnetic Stars;
- Oscillations;
- Stellar Models;
- Stellar Rotation;
- Vibration Mode;
- Splitting;
- Stellar Magnetic Fields;
- Astrophysics