Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..54..445m&link_type=abstract
Astrophysics and Space Science, vol. 54, no. 2, Apr. 1978, p. 445-452.
Astronomy and Astrophysics
Astrophysics
3
Magnetic Field Configurations, Periodic Variations, Perturbation Theory, Stellar Magnetic Fields, Stellar Models, Magnetic Dipoles, Main Sequence Stars, Oscillations
Scientific paper
A first-order perturbation theory method developed by Goossens to
determine the perturbation to the eigenfrequencies of stellar models
caused by the presence of a magnetic field is modified slightly, and
applied to models with toroidal and poloidal fields. Some limitations of
the analysis are pointed out.
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