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dc.contributor.authorBlomme R.
dc.contributor.authorMahy L.
dc.contributor.authorCatala C.
dc.contributor.authorCuypers J.
dc.contributor.authorGosset E.
dc.contributor.authorGodart M.
dc.contributor.authorMontalban J.
dc.contributor.authorVentura P.
dc.contributor.authorRauw G.
dc.contributor.authorMorel T.
dc.contributor.authorDegroote P.
dc.contributor.authorAerts C.
dc.contributor.authorNoels A.
dc.contributor.authorMichel E.
dc.contributor.authorBaudin F.
dc.contributor.authorBaglin A.
dc.contributor.authorAuvergne M.
dc.contributor.authorSamadi R.
dc.date9/2011
dc.date.accessioned2016-04-13T10:04:28Z
dc.date.available2016-04-13T10:04:28Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3561
dc.descriptionhttp://esoads.eso.org/abs/2011A%26A...533A...4B
dc.languageeng
dc.rightsRestricted Access
dc.titleVariability in the CoRoT photometry of three hot O-type stars. HD 46223, HD 46150, and HD 46966
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAstronomy and Astrophysics
dc.source.volume533
dc.source.pageA4
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/0004-6361/201116949
dc.identifier.urlhttp://esoads.eso.org/abs/2011A%26A...533A...4B
dc.source.editorEDP Sciences


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