Show simple item record

dc.contributor.authorCarolan, P. B.
dc.contributor.authorKhanzadyan, T.
dc.contributor.authorRedman, M. P.
dc.contributor.authorThompson, M. A.
dc.contributor.authorJones, P. A.
dc.contributor.authorCunningham, M. R.
dc.contributor.authorLoughnane, R. M.
dc.contributor.authorBains, I.
dc.contributor.authorKeto, E.
dc.date.accessioned2018-09-20T16:02:47Z
dc.date.available2018-09-20T16:02:47Z
dc.date.issued2009-11-21
dc.identifier.citationCarolan, P. B. Khanzadyan, T.; Redman, M. P.; Thompson, M. A.; Jones, P. A.; Cunningham, M. R.; Loughnane, R. M.; Bains, I.; Keto, E. (2009). Supersonic turbulence in the cold massive core jcmt 18354���0649s���. Monthly Notices of the Royal Astronomical Society 400 (1), 78-89
dc.identifier.issn0035-8711,1365-2966
dc.identifier.urihttp://hdl.handle.net/10379/10704
dc.description.abstractAn example of a cold massive core, JCMT 18354-0649S which is a possible high-mass analogue to a low-mass star-forming core, is studied. Line and continuum observations from James Clerk Maxwell Telescope, Mopra Telescope and Spitzer are presented and modelled in detail using a 3D molecular line radiative transfer code. In almost every way, JCMT 18354-0649S is a scaled-up version of a typical low-mass core with similar temperatures, chemical abundances and densities. The difference is that both the infall velocity and the turbulent width of the line profiles are an order of magnitude larger. While the higher infall velocity is expected due to the large mass of JCMT 18354-0649S, we suggest that the dissipation of this highly supersonic turbulence may lead to the creation of dense clumps of gas that surround the high-mass core.
dc.publisherOxford University Press (OUP)
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Ireland
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/3.0/ie/
dc.subjectradiative transfer
dc.subjectstars: formation
dc.subjectism: individual: jcmt 18354-0649s
dc.subjectism: jets and outflows
dc.subjectism: kinematics and dynamics
dc.subjectism: abundances
dc.subjectstar-formation regions
dc.subjectyoung stellar objects
dc.subjectinfrared dark clouds
dc.subjectinitial conditions
dc.subjectmolecular gas
dc.subjectbrown dwarf
dc.subjectradiative-transfer
dc.subjectfreeze-out
dc.subjectoutflow
dc.subjectemission
dc.titleSupersonic turbulence in the cold massive core jcmt 18354���0649s���
dc.typeArticle
dc.identifier.doi10.1111/j.1365-2966.2009.15441.x
dc.local.publishedsourcehttps://academic.oup.com/mnras/article-pdf/400/1/78/18690909/mnras0400-0078.pdf
nui.item.downloads0


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

Attribution-NonCommercial-NoDerivs 3.0 Ireland
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Ireland