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dc.contributor.authorMichel, Eric-
dc.contributor.authorBaglin, Annie-
dc.contributor.authorAuvergne, Michel-
dc.contributor.authorCatala, Claude-
dc.contributor.authorSamadi, Reza-
dc.contributor.authorBaudin, Frédéric-
dc.contributor.authorAppourchaux, Thierry-
dc.contributor.authorBarban, Caroline-
dc.contributor.authorWeiss, Werner W.-
dc.contributor.authorBerthomieu, Gabrielle-
dc.contributor.authorBoumier, Patrick-
dc.contributor.authorDupret, Marc-Antoine-
dc.contributor.authorGarcía, Rafael A.-
dc.contributor.authorFridlund, Malcolm-
dc.contributor.authorGarrido, Rafael-
dc.contributor.authorGoupil, Marie-Jose-
dc.contributor.authorKjeldsen, Hans-
dc.contributor.authorLebreton, Yveline-
dc.contributor.authorMosser, Benoît-
dc.contributor.authorGrotsch-Noels, Arlette-
dc.contributor.authorJanot-Pacheco, Eduardo-
dc.contributor.authorProvost, Janine-
dc.contributor.authorRoxburgh, Ian W.-
dc.contributor.authorThoul, Anne-
dc.contributor.authorToutain, Thierry-
dc.contributor.authorTiphène, Didier-
dc.contributor.authorTurck-Chieze, Sylvaine-
dc.contributor.authorVauclair, Sylvie D.-
dc.contributor.authorVauclair, Gérard P.-
dc.contributor.authorAerts, Conny-
dc.contributor.authorAlecian, Georges-
dc.contributor.authorBallot, Jérôme-
dc.contributor.authorCharpinet, Stéphane-
dc.contributor.authorHubert, Anne-Marie-
dc.contributor.authorLignières, François-
dc.contributor.authorMathias, Philippe-
dc.contributor.authorMonteiro, Mario J.P.F.G.-
dc.contributor.authorNeiner, Coralie-
dc.contributor.authorPoretti, Ennio-
dc.contributor.authorMedeiros, José Renan de-
dc.contributor.authorRibas, Ignasi-
dc.contributor.authorRieutord, Michel L.-
dc.contributor.authorRoca Cortés, Teodoro-
dc.contributor.authorZwintz, Konstanze-
dc.date.accessioned2008-10-24T10:57:34Z-
dc.date.available2008-10-24T10:57:34Z-
dc.date.issued2008-10-24-
dc.identifier.citationScience 322(5901): 558-560 (2008)en_US
dc.identifier.issn0036-8075-
dc.identifier.urihttp://hdl.handle.net/10261/7982-
dc.description4 pages, 3 figures.-- Supporting Online Material: Text, Fig. S1, Table S1 and References, available at: http://www.sciencemag.org/cgi/content/full/322/5901/558/DC1en_US
dc.description.abstractOscillations of the Sun have been used to understand its interior structure. The extension of similar studies to more distant stars has raised many difficulties despite the strong efforts of the international community over the past decades. The CoRoT (Convection Rotation and Planetary Transits) satellite, launched in December 2006, has now measured oscillations and the stellar granulation signature in three main sequence stars that are noticeably hotter than the sun. The oscillation amplitudes are about 1.5 times as large as those in the Sun; the stellar granulation is up to three times as high. The stellar amplitudes are about 25% below the theoretic values, providing a measurement of the nonadiabaticity of the process ruling the oscillations in the outer layers of the stars.en_US
dc.format.extent319019 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherAmerican Association for the Advancement of Scienceen_US
dc.rightsclosedAccessen_US
dc.subjectSolar-Like Oscillationsen_US
dc.subjectStellar granulationen_US
dc.subjectStars hotter than the sunen_US
dc.subjectCoRoT (Convection Rotation and Planetary Transits) satelliteen_US
dc.subjectAsteroseismology-
dc.subjectAstrophysics-
dc.titleCoRoT Measures Solar-Like Oscillations and Granulation in Stars Hotter Than the Sunen_US
dc.typeartículoen_US
dc.identifier.doi10.1126/science.1163004-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1126/science.1163004en_US
dc.identifier.e-issn1095-9203-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairetypeartículo-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
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