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The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase

dc.contributor.authorChesneau O.
dc.contributor.authorMeilland A.
dc.contributor.authorChapellier E.
dc.contributor.authorMillour F.
dc.contributor.authorvan Genderen A. M.
dc.contributor.authorNazé Y.
dc.contributor.authorSmith N.
dc.contributor.authorSpang A.
dc.contributor.authorSmoker J. V.
dc.contributor.authorDessart L.
dc.contributor.authorKanaan S.
dc.contributor.authorBendjoya P.
dc.contributor.authorFeast M. W.
dc.contributor.authorGroh J. H.
dc.contributor.authorLobel A.
dc.contributor.authorNardetto N.
dc.contributor.authorOtero S.
dc.contributor.authorOudmaijer R. D.
dc.contributor.authorTekola A. G.
dc.contributor.authorWhitelock P. A.
dc.contributor.authorArcos C.
dc.contributor.authorCuré M.
dc.contributor.authorVanzi L.
dc.date3/2014
dc.date.accessioned2016-04-13T10:05:37Z
dc.date.available2016-04-13T10:05:37Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3879
dc.descriptionhttp://esoads.eso.org/abs/2014A%26A...563A..71C
dc.languageeng
dc.rightsRestricted Access
dc.titleThe yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAstronomy and Astrophysics
dc.source.volume563
dc.source.pageA71
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/0004-6361/201322421
dc.identifier.urlhttp://esoads.eso.org/abs/2014A%26A...563A..71C
dc.source.editorEDP Sciences


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