Pulsations, chemical composition and multiplicity in main-sequence A- and F-type stars

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dc.creatorHekker, S.
dc.creatorFrémat, Y.
dc.creatorLampens, P.
dc.creatorDe Cat, P.
dc.date2009-01-20
dc.date.accessioned2026-07-07T12:32:28Z
dc.date.available2026-07-07T12:32:28Z
dc.descriptionThe region in the HR-diagram where the main sequence intersects the classical instability strip hosts A- and F-type stars exhibiting a rich variety of physical phenomena, such as pulsations on various time scales and chemical peculiarities. We aim to investigate the occurrence of these phenomena among suspected binary systems in this region of the HR-diagram and their mutual interactions.
dc.descriptionContribution to the Proceedings of the Wroclaw HELAS Workshop, 2008, to appear in Communications in Asterseismology, 157
dc.identifierhttps://arxiv.org/abs/0901.3162
dc.identifierhttp://arxiv.org/abs/0901.3162
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216793
dc.subjectSolar and Stellar Astrophysics
dc.titlePulsations, chemical composition and multiplicity in main-sequence A- and F-type stars
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