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dc.contributor.authorde Villiers, H. M.
dc.contributor.authorThompson, M. A.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorvan der Walt, D. J.
dc.contributor.editorBooth, R. S.
dc.contributor.editorHumphreys, E. M. L.
dc.contributor.editorVlemmings, W. H. T.
dc.date.accessioned2013-05-24T14:00:10Z
dc.date.available2013-05-24T14:00:10Z
dc.date.issued2012-07-01
dc.identifier.citationde Villiers , H M , Thompson , M A , Chrysostomou , A & van der Walt , D J 2012 , Molecular outflows toward methanol masers : detection techniques and their properties . in R S Booth , E M L Humphreys & W H T Vlemmings (eds) , Cosmic Masers : from OH to H0 . Procs of the International Astronomical Union , no. S287 , vol. 8 , Cambridge University Press , pp. 194-195 . https://doi.org/10.1017/S1743921312006965
dc.identifier.otherPURE: 1214522
dc.identifier.otherPURE UUID: 5c38105a-41e5-4193-9662-cbfe8e3aedb6
dc.identifier.otherBibtex: urn:1720aa4206c596e00481bd345a3a1351
dc.identifier.otherScopus: 84864453438
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970799
dc.identifier.urihttp://hdl.handle.net/2299/10676
dc.description.abstractClass II methanol masers are thought to trace the brief phase in the evolution of a massive YSO, where outflows are expected to occur. Molecular line maps of the CO isotopes of a subset of 6.7 GHz sources from the MMB catalogue were observed with the JCMT telescope. Utilising optically thick 12CO, a search was done to detect broadened line wings (initially only on the source G20.08-0.13). The physical parameters of these detected lobes were then calculateden
dc.format.extent2
dc.language.isoeng
dc.publisherCambridge University Press
dc.relation.ispartofCosmic Masers
dc.relation.ispartofseriesProcs of the International Astronomical Union
dc.titleMolecular outflows toward methanol masers : detection techniques and their propertiesen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2012-07-01
rioxxterms.versionofrecordhttps://doi.org/10.1017/S1743921312006965
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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