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dc.contributor.authorBuckle, JV
dc.contributor.authorDrabek-Maunder, E
dc.contributor.authorGreaves, J
dc.contributor.authorRicher, JS
dc.contributor.authorMatthews, BC
dc.contributor.authorJohnstone, D
dc.contributor.authorKirk, H
dc.contributor.authorBeaulieu, SF
dc.contributor.authorBerry, DS
dc.contributor.authorBroekhoven-Fiene, H
dc.contributor.authorCurrie, MJ
dc.contributor.authorFich, M
dc.contributor.authorHatchell, J
dc.contributor.authorJenness, T
dc.contributor.authorMottram, JC
dc.contributor.authorNutter, D
dc.contributor.authorPattle, K
dc.contributor.authorPineda, JE
dc.contributor.authorSalji, C
dc.contributor.authorTisi, S
dc.contributor.authorFrancesco, JD
dc.contributor.authorHogerheijde, MR
dc.contributor.authorWard-Thompson, D
dc.contributor.authorBastien, P
dc.contributor.authorButner, H
dc.contributor.authorChen, M
dc.contributor.authorChrysostomou, A
dc.contributor.authorCoude, S
dc.contributor.authorDavis, CJ
dc.contributor.authorDuarte-Cabral, A
dc.contributor.authorFriberg, P
dc.contributor.authorFriesen, R
dc.contributor.authorFuller, GA
dc.contributor.authorGraves, S
dc.contributor.authorGregson, J
dc.contributor.authorHolland, W
dc.contributor.authorJoncas, G
dc.contributor.authorKirk, JM
dc.contributor.authorKnee, LBG
dc.contributor.authorMairs, S
dc.contributor.authorMarsh, K
dc.contributor.authorMoriarty-Schieven, G
dc.contributor.authorRawlings, J
dc.contributor.authorRosolowsky, E
dc.contributor.authorRumble, D
dc.contributor.authorSadavoy, S
dc.contributor.authorThomas, H
dc.contributor.authorTothill, N
dc.contributor.authorViti, S
dc.contributor.authorWhite, GJ
dc.contributor.authorWilson, CD
dc.contributor.authorWouterloot, J
dc.contributor.authorYates, J
dc.contributor.authorZhu, M
dc.date.accessioned2016-02-29T16:07:45Z
dc.date.issued2015-05-01
dc.description.abstractWe present 850 and 450 μm data from the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey obtained with Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and characterize the dust attributes of Class I, Class II and Class III disc sources in L 1495. We detect 23 per cent of the sample at both wavelengths, with the detection rate decreasing through the Classes from I to III. The median disc mask is 1.6 × 10<SUP>-3</SUP> M<SUB>⊙</SUB>, and only 7 per cent of Class II sources have disc masses larger than 20 Jupiter masses. We detect a higher proportion of discs towards sources with stellar hosts of spectral type K than spectral type M. Class II discs with single stellar hosts of spectral type K have higher masses than those of spectral type M, supporting the hypothesis that higher mass stars have more massive discs. Variations in disc masses calculated at the two wavelengths suggest that there may be differences in dust opacity and/or dust temperature between discs with hosts of spectral types K to those with spectral type M.en_GB
dc.identifier.citationVol. 449, pp. 2472 - 2488en_GB
dc.identifier.doi10.1093/mnras/stv438
dc.identifier.urihttp://hdl.handle.net/10871/20275
dc.language.isoenen_GB
dc.publisherOxford Journalsen_GB
dc.relation.urlhttp://esoads.eso.org/abs/2015MNRAS.449.2472Ben_GB
dc.relation.urlhttp://arxiv.org/abs/1502.07946en_GB
dc.subjectstars: formationen_GB
dc.subjectstars: low massen_GB
dc.subjectsubmillimetre: ISMen_GB
dc.titleThe JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar discs in L 1495en_GB
dc.typeArticleen_GB
dc.date.available2016-02-29T16:07:45Z
dc.identifier.issn0035-8711
dc.descriptionJOURen_GB
dc.descriptionThis is the final version of the article. It was first published by Oxford Journals for the Royal Astronomical Society via http://dx.doi.org/10.1093/mnras/stv438en_GB
dc.identifier.journalMonthly Notices of the Royal Astronomical Societyen_GB


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