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dc.contributor.authorSódor Á.
dc.contributor.authorChené A.-N.
dc.contributor.authorDe Cat P.
dc.contributor.authorBognár Z.
dc.contributor.authorWright D. J.
dc.contributor.authorMarois C.
dc.contributor.authorWalker G. A. H.
dc.contributor.authorMatthews J. M.
dc.contributor.authorKallinger T.
dc.contributor.authorRowe J. F.
dc.contributor.authorKuschnig R.
dc.contributor.authorGuenther D. B.
dc.contributor.authorMoffat A. F. J.
dc.contributor.authorRucinski S. M.
dc.contributor.authorSasselov D.
dc.contributor.authorWeiss W. W.
dc.date8/2014
dc.date.accessioned2016-04-13T10:05:36Z
dc.date.available2016-04-13T10:05:36Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3854
dc.descriptionhttp://esoads.eso.org/abs/2014A%26A...568A.106S
dc.languageeng
dc.rightsRestricted Access
dc.titleMOST light-curve analysis of the γ Doradus pulsator HR 8799, showing resonances and amplitude variations
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAstronomy and Astrophysics
dc.source.volume568
dc.source.pageA106
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/0004-6361/201423976
dc.identifier.urlhttp://esoads.eso.org/abs/2014A%26A...568A.106S
dc.source.editorEDP Sciences


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