Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-08-31
Mon.Not.Roy.Astron.Soc.322:389,2001
Astronomy and Astrophysics
Astrophysics
7 pages, 10 figures, submitted to MNRAS. (revisions: new results are presented)
Scientific paper
10.1046/j.1365-8711.2001.04115.x
By using the Cowling approximation, quasi-radial modes of rotating general relativistic stars are computed along equilibrium sequences from non-rotating to maximally rotating models. The eigenfrequencies of these modes are decreasing functions of the rotational frequency. The eigenfrequency curve of each mode as a function of the rotational frequency has discontinuities, which arise from the avoided crossing with other curves of axisymmetric modes.
Eriguchi Yoshiharu
Yoshida S'i.
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