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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.rightsOpen
dc.titleIs the Outflow from RT Vir Bipolar or Rotatingen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2000
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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