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dc.contributor.authorTedds, J.A.
dc.contributor.authorBrand, P.W.J.L.
dc.contributor.authorBurton, M.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorFernandes, A.J.L.
dc.date.accessioned2008-09-24T08:55:40Z
dc.date.available2008-09-24T08:55:40Z
dc.date.issued1994
dc.identifier.citationTedds , J A , Brand , P W J L , Burton , M , Chrysostomou , A & Fernandes , A J L 1994 , The Physics of Shocked Outflows In Star Forming Molecular Clouds . in In: Procs of Clouds, Cores, and Low Mass Stars - ASP Conf Series 65 . Astronomical Society of the Pacific , pp. 375-379 .
dc.identifier.isbn978-1-58381-401-7
dc.identifier.isbn0-937707-84-8
dc.identifier.otherPURE: 174884
dc.identifier.otherPURE UUID: e4d4523b-208a-4ba9-99e5-c23db5925165
dc.identifier.otherdspace: 2299/2391
dc.identifier.urihttp://hdl.handle.net/2299/2391
dc.descriptionOriginal paper can be found at: http://astrosociety.org/pubs/cs/035-069.html Copyright ASP
dc.description.abstractRecent near-IR imaging of the Orion molecular cloud has revealed a complex of dense bullets, visible as [FeII] emitting HH-objects at the tips of H2 wakes, ejected explosively from the cloud core. Having resolved individual bow-shock structures for the first time in this bright source, we have observed [FeII] 1.644um velocity profiles of selected bullets and H2 1-0 S(1), 2.122um velocity profiles for a series of positions along and across the corresponding bow-shock wakes. We present observed profiles for the bullet M42 HH1 and its associated wake and compare with theoretical bow-shock models.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Clouds, Cores, and Low Mass Stars - ASP Conf Series 65
dc.rightsOpen
dc.titleThe Physics of Shocked Outflows In Star Forming Molecular Cloudsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1994
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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