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Paper: Pulsation Modes with High Azimuthal Orders in Stellar Models Based on the Self-Consistent Field Method
Volume: 416, Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21
Page: 395
Authors: Reese, D. R.; MacGregor, K. B.; Jackson, S.; Skumanich, A.; Metcalfe, T. S.
Abstract: We investigate pulsation modes with high azimuthal orders in a uniformly and differentially rotating stellar model based on the SCF method. Our results show a more complicated m dependence of the pulsation frequencies than what was proposed in previous studies. These results allow a more precise determination of the effects of rapid uniform or differential rotation on stellar pulsations thereby providing a better understanding of the underlying physics.
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