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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.titleThe Physics of Shocked Outflows In Star Forming Molecular Cloudsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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