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dc.contributor.authorCernicharo J.
dc.contributor.authorTeyssier D.
dc.contributor.authorQuintana-Lacaci G.
dc.contributor.authorDaniel F.
dc.contributor.authorAgúndez M.
dc.contributor.authorVelilla-Prieto L.
dc.contributor.authorDecin L.
dc.contributor.authorGuélin M.
dc.contributor.authorEncrenaz P.
dc.contributor.authorGarcía-Lario P.
dc.contributor.authorde Beck E.
dc.contributor.authorBarlow M. J.
dc.contributor.authorGroenewegen M. A. T.
dc.contributor.authorNeufeld D.
dc.contributor.authorPearson J.
dc.date11/2014
dc.date.accessioned2016-04-13T10:05:35Z
dc.date.available2016-04-13T10:05:35Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3830
dc.descriptionhttp://esoads.eso.org/abs/2014ApJ...796L..21C
dc.languageeng
dc.rightsRestricted Access
dc.titleDiscovery of Time Variation of the Intensity of Molecular Lines in IRC+10216 in the Submillimeter and Far-Infrared Domains
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleThe Astrophysical Journal
dc.source.volume796
dc.source.pageL21
Orfeo.peerreviewedYes
dc.identifier.doi10.1088/2041-8205/796/1/L21
dc.identifier.urlhttp://esoads.eso.org/abs/2014ApJ...796L..21C
dc.source.editorIOP


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