Solar-like oscillations in red giants in the CoRoT exo-field

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dc.creatorHekker, S.
dc.creatorBarban, C.
dc.creatorKallinger, T.
dc.creatorWeiss, W.
dc.creatorDe Ridder, J.
dc.creatorHatzes, A.
dc.creatorteam, CoRoT
dc.date2008-10-15
dc.date.accessioned2026-07-07T10:10:34Z
dc.date.available2026-07-07T10:10:34Z
dc.descriptionAsteroseismic observations from space can provide us with long time series of uninterrupted high quality data for many stars at the same time. The CoRoT satellite (Convection Rotation and planetary Transits) was launched successfully in December 2006 and provides high precision photometery for a large number of stars. Here we present our research on (late G and K) red giant stars observed during the first long run (150 days) of CoRoT with the 'eye' dedicated to exo-planet research.
dc.description2 pages, 1 figure, contribution to the Proceedings of the Wroclaw HELAS Workshop, 2008, to be published in Communications in Asteroseismology
dc.identifierhttps://arxiv.org/abs/0810.2797
dc.identifierhttp://arxiv.org/abs/0810.2797
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/171635
dc.subjectAstrophysics
dc.titleSolar-like oscillations in red giants in the CoRoT exo-field
dc.typetext

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