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The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP

dc.contributor.authorGraves, S. F.
dc.contributor.authorRicher, J. S.
dc.contributor.authorBuckle, J. V.
dc.contributor.authorDuarte-Cabral, A.
dc.contributor.authorFuller, G. A.
dc.contributor.authorHogerheijde, M. R.
dc.contributor.authorOwen, J. E.
dc.contributor.authorBrunt, C.
dc.contributor.authorButner, H. M.
dc.contributor.authorCavanagh, B.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorCurtis, E. I.
dc.contributor.authorDavis, C. J.
dc.contributor.authorEtxaluze, M.
dc.contributor.authorDi Francesco, J.
dc.contributor.authorFriberg, P.
dc.contributor.authorFriesen, R. K.
dc.contributor.authorGreaves, J. S.
dc.contributor.authorHatchell, J.
dc.contributor.authorJohnstone, D.
dc.contributor.authorMatthews, B.
dc.contributor.authorMatthews, H.
dc.contributor.authorMatzner, C. D.
dc.contributor.authorNutter, D.
dc.contributor.authorRawlings, J. M. C.
dc.contributor.authorRoberts, J. F.
dc.contributor.authorSadavoy, S.
dc.contributor.authorSimpson, R. J.
dc.contributor.authorTothill, N. F. H.
dc.contributor.authorTsamis, Y. G.
dc.contributor.authorViti, S.
dc.contributor.authorWard-Thompson, D.
dc.contributor.authorWhite, G. J.
dc.contributor.authorWouterloot, J. G. A.
dc.contributor.authorYates, J.
dc.date.accessioned2011-10-20T10:01:11Z
dc.date.available2011-10-20T10:01:11Z
dc.date.issued2010-12-21
dc.identifier.citationGraves , S F , Richer , J S , Buckle , J V , Duarte-Cabral , A , Fuller , G A , Hogerheijde , M R , Owen , J E , Brunt , C , Butner , H M , Cavanagh , B , Chrysostomou , A , Curtis , E I , Davis , C J , Etxaluze , M , Di Francesco , J , Friberg , P , Friesen , R K , Greaves , J S , Hatchell , J , Johnstone , D , Matthews , B , Matthews , H , Matzner , C D , Nutter , D , Rawlings , J M C , Roberts , J F , Sadavoy , S , Simpson , R J , Tothill , N F H , Tsamis , Y G , Viti , S , Ward-Thompson , D , White , G J , Wouterloot , J G A & Yates , J 2010 , ' The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP ' , Monthly Notices of the Royal Astronomical Society , vol. 409 , no. 4 , pp. 1412-1428 . https://doi.org/10.1111/j.1365-2966.2010.17140.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 425142
dc.identifier.otherPURE UUID: afe9f060-422a-4cf8-8c3b-455d55722bff
dc.identifier.otherWOS: 000284963800008
dc.identifier.otherScopus: 78650033317
dc.identifier.urihttp://hdl.handle.net/2299/6733
dc.descriptionThe definitive version is found at: http://onlinelibrary.wiley.com Copyright Royal Astronomical Society
dc.description.abstractThe Gould Belt Legacy Survey on the James Clerk Maxwell Telescope's has observed a region of 260 arcmin2 in 12CO J = 3 -> 2 emission, and a 190 arcmin2 subset of this in 13CO and C18O towards the Serpens molecular cloud. We examine the global velocity structure of the non-outflowing gas, and calculate excitation temperatures and opacities. The large-scale mass and energetics of the region are evaluated, with special consideration for high-velocity gas. We find the cloud to have a mass of 203 M-circle dot, and to be gravitationally bound, and that the kinetic energy of the outflowing gas is approximately 70 per cent of the turbulent kinetic energy of the cloud. We identify compact outflows towards some of the submillimetre Class 0/I sources in the region.en
dc.format.extent17
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectmolecular data
dc.subjectstars: formation
dc.subjectISM: jets and outflows
dc.subjectISM: kinematics and dynamics
dc.subjectsubmillimetre: ISM
dc.titleThe JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARPen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2010.17140.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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