A comparison of oscillation frequencies of rotating stars obtained by one- and two-dimensional calculations

Details A comparison of oscillation frequencies of rotating stars obtained by one- and two-dimensional calculations A comparison of oscillation frequencies of rotating stars obtained by one- and two-dimensional calculations

2011-09-12

arxiv.org/abs/1109.2373v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 3 figures; Proceedings of the 61st Fujihara Seminar: Progress in solar/stellar physics with helio- and asteroseismolo

Scientific paper

We discuss how the p- and g-mode frequencies calculated for rotating stars
are affected by the way of including the centrifugal deformations. We find that
p-mode frequencies are sensitive to the accuracy in treating the centrifugal
deformation, while the effect becomes smaller for smaller frequencies in the
g-mode range.

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