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Close binary and other variable stars in the solar-age Galactic open cluster M 67

dc.contributor.authorYakut K.
dc.contributor.authorZima W.
dc.contributor.authorKalomeni B.
dc.contributor.authorvan Winckel H.
dc.contributor.authorWaelkens C.
dc.contributor.authorDe Cat P.
dc.contributor.authorBauwens E.
dc.contributor.authorVučković M.
dc.contributor.authorSaesen S.
dc.contributor.authorLe Guillou L.
dc.contributor.authorParmaksızoğlu M.
dc.contributor.authorUluç K.
dc.contributor.authorKhamitov I.
dc.contributor.authorRaskin G.
dc.contributor.authorAerts C.
dc.date8/2009
dc.date.accessioned2016-04-13T10:04:34Z
dc.date.available2016-04-13T10:04:34Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3713
dc.descriptionhttp://esoads.eso.org/abs/2009A%26A...503..165Y
dc.languageeng
dc.rightsRestricted Access
dc.titleClose binary and other variable stars in the solar-age Galactic open cluster M 67
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleAstronomy and Astrophysics
dc.source.volume503
dc.source.page165
Orfeo.peerreviewedYes
dc.identifier.doi10.1051/0004-6361/200911918
dc.identifier.urlhttp://esoads.eso.org/abs/2009A%26A...503..165Y
dc.source.editorEDP Sciences


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