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dc.contributor.authorSreenilayam, G.
dc.contributor.authorFich, M.
dc.contributor.authorAde, P.
dc.contributor.authorBintley, D.
dc.contributor.authorChapin, E.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorDunlop, J.S.
dc.contributor.authorGibb, A.
dc.contributor.authorGreaves, J.S.
dc.contributor.authorHalpern, M.
dc.contributor.authorHolland, W.S.
dc.contributor.authorIvison, R.
dc.contributor.authorJenness, T.
dc.contributor.authorRobson, I.
dc.contributor.authorScott, D.
dc.identifier.citationSreenilayam , G , Fich , M , Ade , P , Bintley , D , Chapin , E , Chrysostomou , A , Dunlop , J S , Gibb , A , Greaves , J S , Halpern , M , Holland , W S , Ivison , R , Jenness , T , Robson , I & Scott , D 2014 , ' Cold dust in hot regions ' , Astronomical Journal , vol. 147 , no. 3 .
dc.descriptionThe James Clerk Maxwell Telescope is operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the United Kingdom, the National Research Council of Canada, and (until 2013 March 31) the Netherlands Organisation for Scientific Research. Additional funds for the construction of SCUBA-2 were provided by the Canada Foundation for Innovation.en
dc.description.abstractWe mapped five massive star-forming regions with the SCUBA-2 camera on the James Clerk Maxwell Telescope. Temperature and column density maps are obtained from the SCUBA-2 450 and 850 μm images. Most of the dense clumps we find have central temperatures below 20 K, with some as cold as 8 K, suggesting that they have no internal heating due to the presence of embedded protostars. This is surprising, because at the high densities inferred from these images and at these low temperatures such clumps should be unstable, collapsing to form stars and generating internal heating. The column densities at the clump centers exceed 1023 cm-2, and the derived peak visual extinction values are from 25 to 500 mag for β = 1.5-2.5, indicating highly opaque centers. The observed cloud gas masses range from ~10 to 103 M ☉. The outer regions of the clumps follow an r-2.36±0.35 density distribution, and this power-law structure is observed outside of typically 104 AU. All these findings suggest that these clumps are high-mass starless clumps and most likely contain high-mass starless cores.
dc.relation.ispartofAstronomical Journalen
dc.subjectSubmillimeter: ISMen
dc.subjectStars: formationen
dc.subjectISM: cloudsen
dc.subjectH II regionsen
dc.subjectQB Astronomyen
dc.titleCold dust in hot regionsen
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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