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dc.contributor.authorYates, J.A.
dc.contributor.authorRichards, A.M.S.
dc.contributor.authorGledhill, T.
dc.contributor.authorBains, I.
dc.date.accessioned2008-01-30T10:36:15Z
dc.date.available2008-01-30T10:36:15Z
dc.date.issued2000
dc.identifier.citationYates , J A , Richards , A M S , Gledhill , T & Bains , I 2000 , Is the Outflow from RT Vir Bipolar or Rotating . in In: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199 . Astronomical Society of the Pacific , pp. 79-82 .
dc.identifier.isbn1-58381-026-9
dc.identifier.otherPURE: 143090
dc.identifier.otherPURE UUID: 97322198-d7f0-4177-b000-e17f47c4bd68
dc.identifier.otherdspace: 2299/1440
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779795
dc.identifier.urihttp://hdl.handle.net/2299/1440
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/195-221.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present high angular resolution observations of H2O maser proper motions in the circumstellar envelope of the semi-regular variable RT Vir. The MERLIN observations, at 12-mas angular resolution, were used to map H2O maser emission at ~2 week intervals over 10 weeks in 1996, during which period the brightness distribution changed markedly.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199
dc.titleIs the Outflow from RT Vir Bipolar or Rotatingen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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