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2D non-perturbative modeling of oscillations in rapidly rotating stars

We present and discuss results of a recently developped two dimensional non-perturbative method to compute accurate adiabatic oscillation modes of rapidly rotating stars . The 2D calculations fully take into account the centrifugal distorsion of the star while the non-perturbative method includes the full influence of the Coriolis acceleration. These characteristics allows us to compute oscillation modes of rapid rotators - from high order p-modes in $δ$Scuti stars, to low order p- and g-modes in $β$ Cephei or Be stars.

preprint2013arXivOpen access
R-M. OuazzaniM-A. DupretM. J. GoupilD. R. Reese
astro-ph.SR
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Open access4 authors1 topic
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R-M. OuazzaniM-A. DupretM. J. GoupilD. R. Reese

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