Asteroseismology and forced oscillations of HD 209295, the first member of two classes of pulsating star

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dc.creatorHandler, G.
dc.creatorBalona, L. A.
dc.creatorShobbrook, R. R.
dc.creatorKoen, C.
dc.creatorBruch, A.
dc.creatorRomero-Colmenero, E.
dc.creatorPamyatnykh, A. A.
dc.creatorWillems, B.
dc.creatorEyer, L.
dc.creatorJames, D. J.
dc.creatorMaas, T.
dc.creatorCrause, L. A.
dc.date2001-10-16
dc.date.accessioned2026-07-07T02:00:52Z
dc.date.available2026-07-07T02:00:52Z
dc.descriptionWe report the discovery of both intermediate-order gravity mode and low-order pressure mode pulsation in the same star, HD 209295. It is therefore both a gamma Doradus and a delta Scuti star, which makes it the first confirmed member of two classes of pulsating star. This object is located in a close binary system with an unknown, but likely degenerate companion in an eccentric orbit, and some of the gamma Doradus pulsation frequencies are exact integer multiples of the orbital frequency. We suggest that these pulsations are tidally excited. HD 209295 may be the progenitor of an intermediate-mass X-Ray binary.
dc.description4 pages, 1 figure, to appear in the proceedings of IAU Colloquium 185 "Radial and Nonradial Pulsations as Probes of Stellar physics", C.Aerts, T.Bedding and J.Christensen-Dalsgaard, eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0110389
dc.identifierhttp://arxiv.org/abs/astro-ph/0110389
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3554
dc.subjectAstrophysics
dc.titleAsteroseismology and forced oscillations of HD 209295, the first member of two classes of pulsating star
dc.typetext

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