The numerical determination of the eigenfrequencies of a rotating star

Statistics – Computation

Scientific paper

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Computational Astrophysics, Eigenvectors, Stellar Oscillations, Stellar Rotation, Astronomical Models, Differential Equations, Stellar Mass

Scientific paper

A technique for finding the oscillation spectrum of a rotating star based on the solution of two simultaneous ordinary differential equations is described. Results are presented for some g-modes of the polytrope of index 2. It appears that the functional dependence of frequency on rotational velocity is different for different azimuthal wave numbers m.

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