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Two-dimensional Monte Carlo simulations of H i line formation in massive young stellar object disc winds

dc.contributor.authorSim, S.
dc.contributor.authorDrew, J.E.
dc.contributor.authorLong, K.S.
dc.date.accessioned2008-01-02T10:00:12Z
dc.date.available2008-01-02T10:00:12Z
dc.date.issued2005
dc.identifier.citationSim , S , Drew , J E & Long , K S 2005 , ' Two-dimensional Monte Carlo simulations of H i line formation in massive young stellar object disc winds ' , Monthly Notices of the Royal Astronomical Society , vol. 363 , no. 2 , pp. 615-627 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 144305
dc.identifier.otherPURE UUID: ce1557f2-786c-434a-8f52-c899e305b5d8
dc.identifier.otherdspace: 2299/1285
dc.identifier.otherScopus: 27144540471
dc.identifier.urihttp://hdl.handle.net/2299/1285
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleTwo-dimensional Monte Carlo simulations of H i line formation in massive young stellar object disc windsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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