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Mass ratio from Doppler beaming and Rømer delay versus ellipsoidal modulation in the Kepler data of KOI-74

dc.contributor.authorBloemen S.
dc.contributor.authorMarsh T. R.
dc.contributor.authorDegroote P.
dc.contributor.authorØstensen R. H.
dc.contributor.authorPápics P. I.
dc.contributor.authorAerts C.
dc.contributor.authorKoester D.
dc.contributor.authorGänsicke B. T.
dc.contributor.authorBreedt E.
dc.contributor.authorLombaert R.
dc.contributor.authorPyrzas S.
dc.contributor.authorCopperwheat C. M.
dc.contributor.authorExter K.
dc.contributor.authorRaskin G.
dc.contributor.authorVan Winckel H.
dc.contributor.authorPrins S.
dc.contributor.authorPessemier W.
dc.contributor.authorFrémat Y.
dc.contributor.authorHensberge H.
dc.contributor.authorJorissen A.
dc.contributor.authorVan Eck S.
dc.date5/2012
dc.date.accessioned2016-04-13T10:04:26Z
dc.date.available2016-04-13T10:04:26Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3500
dc.descriptionhttp://esoads.eso.org/abs/2012MNRAS.422.2600B
dc.languageeng
dc.rightsRestricted Access
dc.titleMass ratio from Doppler beaming and Rømer delay versus ellipsoidal modulation in the Kepler data of KOI-74
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleMonthly Notices of the Royal Astronomical Society
dc.source.volume422
dc.source.page2600
Orfeo.peerreviewedYes
dc.identifier.doi10.1111/j.1365-2966.2012.20818.x
dc.identifier.urlhttp://esoads.eso.org/abs/2012MNRAS.422.2600B
dc.source.editorWILEY


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