dc.contributor.author | Parsons, H. | |
dc.contributor.author | Thompson, M.A. | |
dc.contributor.author | Clark, J.S. | |
dc.contributor.author | Chrysostomou, A. | |
dc.date.accessioned | 2013-03-14T13:39:46Z | |
dc.date.available | 2013-03-14T13:39:46Z | |
dc.date.issued | 2012-08-01 | |
dc.identifier.citation | Parsons , 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.issn | 0035-8711 | |
dc.identifier.other | PURE: 1213889 | |
dc.identifier.other | PURE UUID: bcffa24c-f09f-4005-95b8-29becff798bf | |
dc.identifier.other | Bibtex: urn:358562bed4c01c466866ff83c761cbfa | |
dc.identifier.other | Scopus: 84864515262 | |
dc.identifier.other | ORCID: /0000-0001-5392-909X/work/30970798 | |
dc.identifier.uri | http://hdl.handle.net/2299/10153 | |
dc.description | full text copy not available in arXiv | |
dc.description.abstract | In 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 GMC | en |
dc.format.extent | 14 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | Molecular clumps in the W51 giant molecular cloud | en |
dc.contributor.institution | Science & Technology Research Institute | |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | https://doi.org/10.1111/j.1365-2966.2012.21106.x | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |