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dc.contributor.authorBains, I.
dc.contributor.authorYates, J.A.
dc.contributor.authorGledhill, T.
dc.contributor.authorRichards, A.M.S.
dc.date.accessioned2010-02-15T12:26:24Z
dc.date.available2010-02-15T12:26:24Z
dc.date.issued2003
dc.identifier.citationBains , I , Yates , J A , Gledhill , T & Richards , A M S 2003 , ' The disappearance of the 1667-MHz OH maser in IRAS 17436+5003 (HD 161796) ' , Monthly Notices of the Royal Astronomical Society , vol. 346 , no. 3 , pp. L46-L50 . https://doi.org/10.1111/j.1365-2966.2003.07334.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 154416
dc.identifier.otherPURE UUID: 6cbd383f-6ebc-4f92-b0fc-4e56e1f470ca
dc.identifier.otherdspace: 2299/4272
dc.identifier.otherScopus: 0348158229
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779779
dc.identifier.urihttp://hdl.handle.net/2299/4272
dc.description‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1365-2966.2003.07334.x [Full text of this article is not available in the UHRA]
dc.description.abstractWe report the diminution of the 1667-MHz OH maser in the post-asymptotic giant branch star IRAS 17436+5003, by a factor of ≳17 over a period of ≲12 yr, from observations with MERLIN. This circumstellar maser was detected by Likkel in 1987, at the 13σ level of her observations with the Green Bank Telescope. We discuss a number of possible reasons for this phenomenon and conclude that it is most likely due to turbulence arising from interacting stellar winds.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleThe disappearance of the 1667-MHz OH maser in IRAS 17436+5003 (HD 161796)en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2003.07334.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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