Oscillations of rapidly rotating stars

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dc.creatorDintrans, Boris
dc.creatorRieutord, Michel
dc.date2001-11-23
dc.date.accessioned2026-07-07T02:01:29Z
dc.date.available2026-07-07T02:01:29Z
dc.descriptionWe present numerical simulations of gravito-inertial waves propagating in radiative zones of rapidly rotating stars. A first model, using the Boussinesq approximation, allows us to study the oscillations of a quasi-incompressible stratified fluid embedded in a rapidly rotating sphere or spherical shell. In a second step, we investigate the case of a Gamma-Doradus star using the anelastic approximation. Some fascinating features of rapidly rotating fluids, such as wave attractors, appear in both cases.
dc.descriptionIAU176 proceedings ``The Impact of Large-Scale Surveys on Pulsating Star Research'', L. Szabados and D. Kurtz (eds.), ASP Conference Series, Vol. 203, 373 (2000)
dc.identifierhttps://arxiv.org/abs/astro-ph/0111453
dc.identifierhttp://arxiv.org/abs/astro-ph/0111453
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3764
dc.subjectAstrophysics
dc.titleOscillations of rapidly rotating stars
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