Effect of rotational and tidal distortions on the periods of small adiabatic oscillations of stellar models

Details Effect of rotational and tidal distortions on the periods of small adiabatic oscillations of stellar models Effect of rotational and tidal distortions on the periods of small adiabatic oscillations of stellar models

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85...83m&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 83-98.

Astronomy and Astrophysics

Astrophysics

6

Stellar Models, Stellar Oscillations, Stellar Rotation, Stellar Structure, Tides, Adiabatic Conditions, Spheres

Scientific paper

Kopal's method of representing the inner structure of a rotationally- and tidally-distorted star by a rotationally- and tidally-distorted Roche model has been used in conjunction with an averaging concept introduced by Kippenhahn and Thomas (1970). According to this concept, the equipotential surfaces of a rotationally- and tidally-distorted stellar model are represented by the equipotential surfaces of an equivalent spherical model. In this way, the combined effects of rotation and tidal distortion on the periods of small adiabatic oscillations of a stellar model are determined.

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