Low Frequency Oscillations of a Slowly Rotating Star - Quasi Toroidal Modes

Details Low Frequency Oscillations of a Slowly Rotating Star - Quasi Toroidal Modes Low Frequency Oscillations of a Slowly Rotating Star - Quasi Toroidal Modes

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94..126p&link_type=abstract

Astronomy and Astrophysics, Vol. 94, P. 126, 1981

Astronomy and Astrophysics

Astrophysics

127

Scientific paper

The radial structure and the frequencies of the nonaxisymmetric
quasi-toroidal modes of a slowly rotating star have been computed in the
case of rigid rotation. The main results are that these modes may have a
significant amplitude in the interior of the star and that they are
greatly influenced by the non-sphericity of the star.

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