Acoustic modes in spheroidal cavities

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dc.creatorLignières, F.
dc.creatorRieutord, M.
dc.creatorValdettaro, L.
dc.date2001-10-09
dc.date.accessioned2026-07-07T02:00:44Z
dc.date.available2026-07-07T02:00:44Z
dc.descriptionOscillation modes of rapidly rotating stars have not yet been calculated with precision, rotational effects being generally approximated by perturbation methods. We are developing a numerical method able to account for the deformation of the star by the centrifugal force and, as a first step, we determined the acoustic modes of a uniform density spheroid and studied how the spheroid flatness affects these modes.
dc.description4 pages, Proceedings of "Semaine de l'Astrophysique Francaise", Edts, SF2A, EdP-Sciences Conf. Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0110214
dc.identifierhttp://arxiv.org/abs/astro-ph/0110214
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3506
dc.subjectAstrophysics
dc.titleAcoustic modes in spheroidal cavities
dc.typetext

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