The Gamma Doradus variables, a new class of pulsating stars. The case of HD 224945

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dc.creatorPoretti, E.
dc.creatorAkan, C.
dc.creatorBossi, M.
dc.creatorKoen, C.
dc.creatorKrisciunas, K.
dc.creatorRodriguez, E.
dc.date1996-12-06
dc.date.accessioned2026-07-07T02:22:28Z
dc.date.available2026-07-07T02:22:28Z
dc.descriptionA multisite campaign involving five observatories allowed us to solve the light curve of the Gamma Doradus star HD 224945. The multiperiodic content, the high frequency term at 3.00 c/d and the frequency spacing between the observed terms strongly support its pulsational nature. Considering the low frequency terms observed in Gamma Dor stars, it seems that g--mode pulsators can be found near the cold border of the instability strip.
dc.description2 pages, latex, 1 figure To be publishing in the Proceedings of the IAU Symposium 181 'Sounding Solar and Stellar Interior', Nice, 30 Sept-3 Oct, 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9612063
dc.identifierhttp://arxiv.org/abs/astro-ph/9612063
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10890
dc.subjectAstrophysics
dc.titleThe Gamma Doradus variables, a new class of pulsating stars. The case of HD 224945
dc.typetext

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