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Modelling a high-mass red giant observed by CoRoT

dc.contributor.authorBaudin F.
dc.contributor.authorBarban C.
dc.contributor.authorGoupil M. J.
dc.contributor.authorSamadi R.
dc.contributor.authorLebreton Y.
dc.contributor.authorBruntt H.
dc.contributor.authorMorel T.
dc.contributor.authorLefèvre L.
dc.contributor.authorMichel E.
dc.contributor.authorMosser B.
dc.contributor.authorCarrier F.
dc.contributor.authorDe Ridder J.
dc.contributor.authorHatzes A.
dc.contributor.authorHekker S.
dc.contributor.authorKallinger T.
dc.contributor.authorAuvergne M.
dc.contributor.authorBaglin A.
dc.contributor.authorCatala C.
dc.date2/2012
dc.date.accessioned2016-04-13T10:04:27Z
dc.date.available2016-04-13T10:04:27Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3525
dc.descriptionhttp://esoads.eso.org/abs/2012A%26A...538A..73B
dc.languageeng
dc.rightsRestricted Access
dc.titleModelling a high-mass red giant observed by CoRoT
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAstronomy and Astrophysics
dc.source.volume538
dc.source.pageA73
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/0004-6361/201116967
dc.identifier.urlhttp://esoads.eso.org/abs/2012A%26A...538A..73B
dc.source.editorEDP Sciences


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