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Herschel SPIRE and PACS observations of the red supergiant VY CMa: analysis of the molecular line spectra

dc.contributor.authorMatsuura M.
dc.contributor.authorYates J. A.
dc.contributor.authorBarlow M. J.
dc.contributor.authorSwinyard B. M.
dc.contributor.authorRoyer P.
dc.contributor.authorCernicharo J.
dc.contributor.authorDecin L.
dc.contributor.authorWesson R.
dc.contributor.authorPolehampton E. T.
dc.contributor.authorBlommaert J. A. D. L.
dc.contributor.authorGroenewegen M. A. T.
dc.contributor.authorVan de Steene G. C.
dc.contributor.authorvan Hoof P. A. M.
dc.date1/2014
dc.date.accessioned2016-04-13T10:05:37Z
dc.date.available2016-04-13T10:05:37Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3887
dc.descriptionhttp://esoads.eso.org/abs/2014MNRAS.437..532M
dc.languageeng
dc.rightsRestricted Access
dc.titleHerschel SPIRE and PACS observations of the red supergiant VY CMa: analysis of the molecular line spectra
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleMonthly Notices of the Royal Astronomical Society
dc.source.volume437
dc.source.page532
Orfeo.peerreviewedYes
dc.identifier.doi10.1093/mnras/stt1906
dc.identifier.urlhttp://esoads.eso.org/abs/2014MNRAS.437..532M
dc.source.editorOUP


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