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Paper: A Comparison of Oscillation Frequencies of Rotating Stars Obtained by One and Two-dimensional Calculations
Volume: 462, Progress in Solar/Stellar Physics with Helio- and Asteroseismology
Page: 398
Authors: Saio, H.; Deupree, R. G.
Abstract: 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 lower frequencies in the g-mode range.
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