dc.contributor.author | Yates, J.A. | |
dc.contributor.author | Richards, A.M.S. | |
dc.contributor.author | Gledhill, T. | |
dc.contributor.author | Bains, I. | |
dc.date.accessioned | 2008-01-30T10:36:15Z | |
dc.date.available | 2008-01-30T10:36:15Z | |
dc.date.issued | 2000 | |
dc.identifier.citation | Yates , 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.isbn | 1-58381-026-9 | |
dc.identifier.other | PURE: 143090 | |
dc.identifier.other | PURE UUID: 97322198-d7f0-4177-b000-e17f47c4bd68 | |
dc.identifier.other | dspace: 2299/1440 | |
dc.identifier.other | ORCID: /0000-0002-2859-4600/work/30779795 | |
dc.identifier.uri | http://hdl.handle.net/2299/1440 | |
dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/195-221.html--Copyright Astronomical Society of the Pacific | |
dc.description.abstract | We 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.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199 | |
dc.title | Is the Outflow from RT Vir Bipolar or Rotating | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |