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dc.contributor.authorDodds, P.
dc.contributor.authorGreaves, J. S.
dc.contributor.authorScholz, A.
dc.contributor.authorHatchell, J.
dc.contributor.authorHolland, W. S.
dc.contributor.authorJCMT Gould Belt Survey Team
dc.date.accessioned2015-02-20T16:31:01Z
dc.date.available2015-02-20T16:31:01Z
dc.date.issued2015-02-11
dc.identifier.citationDodds , P , Greaves , J S , Scholz , A , Hatchell , J , Holland , W S & JCMT Gould Belt Survey Team 2015 , ' The JCMT Gould Belt Survey : low-mass protoplanetary discs from a SCUBA-2 census of NGC 1333 ' , Monthly Notices of the Royal Astronomical Society , vol. 447 , no. 1 , pp. 722-727 . https://doi.org/10.1093/mnras/stu2415en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 162668094
dc.identifier.otherPURE UUID: 22c178c4-bca8-4b24-89d9-b73c24d8dd89
dc.identifier.otherBibCode: 2015MNRAS.447..722D
dc.identifier.otherScopus: 84922426805
dc.identifier.otherWOS: 000350272700057
dc.identifier.urihttp://hdl.handle.net/10023/6130
dc.descriptionDate of Acceptance: 12/11/2014en
dc.description.abstractNGC 1333 is a 1–2 Myr old cluster of stars in the Perseus molecular cloud. We used 850 μm data from the Gould Belt Survey with SCUBA-2 on the James Clerk Maxwell Telescope to measure or place limits on disc masses for 82 Class II sources in this cluster. Eight disc candidates were detected; one is estimated to have mass of about 9 MJup in dust plus gas, while the others host only 2–4 MJup of circumstellar material. None of these discs exceeds the threshold for the ‘minimum mass solar nebula’ (MMSN). This reinforces previous claims that only a small fraction of Class II sources at an age of 1–2 Myr have discs exceeding the MMSN threshold and thus can form a planetary system like our own. However, other regions with similarly low fractions of MMSN discs (IC 348, UpSco, σ Ori) are thought to be older than NGC 1333. Compared with coeval regions, the exceptionally low fraction of massive discs in NGC 1333 cannot easily be explained by the effects of UV radiation or stellar encounters. Our results indicate that additional environmental factors significantly affect disc evolution and the outcome of planet formation by core accretion.
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, © 2014 The Authors, Published by Oxford University Press on behalf of the Royal Astronomical Society.en
dc.subjectPlanets and satellites: formationen
dc.subjectProtoplanetary discsen
dc.subjectStars: formationen
dc.subjectStars: pre-main-sequenceen
dc.subjectQC Physicsen
dc.subjectQB Astronomyen
dc.subject3rd-DASen
dc.subject.lccQCen
dc.subject.lccQBen
dc.titleThe JCMT Gould Belt Survey : low-mass protoplanetary discs from a SCUBA-2 census of NGC 1333en
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stu2415
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2015MNRAS.447..722Den


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