Pulsation Modes with High Azimuthal Orders in Stellar Models Based on the Self-Consistent Field Method

Details Pulsation Modes with High Azimuthal Orders in Stellar Models Based on the Self-Consistent Field Method Pulsation Modes with High Azimuthal Orders in Stellar Models Based on the Self-Consistent Field Method

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..395r&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

Physics

Scientific paper

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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