| dc.contributor.author | Bains, I. | |
| dc.contributor.author | Yates, J.A. | |
| dc.contributor.author | Gledhill, T. | |
| dc.contributor.author | Richards, A.M.S. | |
| dc.date.accessioned | 2010-02-15T12:26:24Z | |
| dc.date.available | 2010-02-15T12:26:24Z | |
| dc.date.issued | 2003 | |
| dc.identifier.citation | Bains , 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.issn | 0035-8711 | |
| dc.identifier.other | dspace: 2299/4272 | |
| dc.identifier.other | ORCID: /0000-0002-2859-4600/work/30779779 | |
| dc.identifier.uri | http://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.abstract | We 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.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | The disappearance of the 1667-MHz OH maser in IRAS 17436+5003 (HD 161796) | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | 10.1111/j.1365-2966.2003.07334.x | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
