Statistics – Computation
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.136...91k&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 136, no. 1, Aug. 1987, p. 91-99.
Statistics
Computation
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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