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dc.contributor.authorParsons, H.
dc.contributor.authorThompson, M.A.
dc.contributor.authorClark, J.S.
dc.contributor.authorChrysostomou, A.
dc.date.accessioned2013-03-14T13:39:46Z
dc.date.available2013-03-14T13:39:46Z
dc.date.issued2012-08-01
dc.identifier.citationParsons , H , Thompson , M A , Clark , J S & Chrysostomou , A 2012 , ' Molecular clumps in the W51 giant molecular cloud ' , Monthly Notices of the Royal Astronomical Society , vol. 424 , no. 3 , pp. 1658-1671 . https://doi.org/10.1111/j.1365-2966.2012.21106.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 1213889
dc.identifier.otherPURE UUID: bcffa24c-f09f-4005-95b8-29becff798bf
dc.identifier.otherBibtex: urn:358562bed4c01c466866ff83c761cbfa
dc.identifier.otherScopus: 84864515262
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970798
dc.identifier.urihttp://hdl.handle.net/2299/10153
dc.descriptionfull text copy not available in arXiv
dc.description.abstractIn this paper, we present a catalogue of dense molecular clumps located within the W51 giant molecular cloud (GMC). This work is based on Heterodyne Array Receiver Programme 13CO J = 3–2 observations of the W51 GMC and uses the automated CLUMPFIND algorithm to decompose the region into a total of 1575 clumps of which 1130 are associated with the W51 GMCen
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleMolecular clumps in the W51 giant molecular clouden
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2012.21106.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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