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dc.contributor.authorFujiyoshi, T.
dc.contributor.authorSmith, C.H.
dc.contributor.authorMoore, T.J.T.
dc.contributor.authorLumsden, S.
dc.contributor.authorAitken, D.
dc.contributor.authorRoche, P.F.
dc.date.accessioned2010-02-18T09:47:45Z
dc.date.available2010-02-18T09:47:45Z
dc.date.issued2005
dc.identifier.citationFujiyoshi , T , Smith , C H , Moore , T J T , Lumsden , S , Aitken , D & Roche , P F 2005 , ' Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2 ' , Monthly Notices of the Royal Astronomical Society , vol. 356 , no. 3 , pp. 801-809 . https://doi.org/10.1111/j.1365-2966.2004.08501.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 177975
dc.identifier.otherPURE UUID: fd438440-3a83-4811-8a4a-31df61bdf677
dc.identifier.otherdspace: 2299/4286
dc.identifier.otherScopus: 12944289540
dc.identifier.urihttp://hdl.handle.net/2299/4286
dc.description‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1365-2966.2004.08501.x [Full text of this article is not available in the UHRA]
dc.description.abstractWe present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6−0.2. The slope of the K-luminosity function towards the region (0.24 ± 0.01) is considered to be equivalent to that expected for main-sequence stars in the solar neighbourhood. Point sources with their (H−K) colour greater than 1 are more likely to be located in extended emission and it is suggested that these objects are physically associated with the H ii region.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleNear-infrared imaging observations of the southern massive star-forming region G333.6-0.2en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2004.08501.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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