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dc.contributor.authorVink, J.S.
dc.contributor.authorDrew, J.E.
dc.contributor.authorHarries, T.J.
dc.contributor.authorOudmaijer, R.D.
dc.date.accessioned2008-02-21T10:53:21Z
dc.date.available2008-02-21T10:53:21Z
dc.date.issued2002
dc.identifier.citationVink , J S , Drew , J E , Harries , T J & Oudmaijer , R D 2002 , Are all Young Stars Disc Accretors . in In: Procs of the Hot Star Workshop III: the Earliest Stages of Massive Star Birth - ASP Conf Series Vol.267 . Astronomical Society of the Pacific , pp. 439-440 .
dc.identifier.isbn978-1-58381-603-5
dc.identifier.isbn1-58381-107-9
dc.identifier.otherPURE: 147298
dc.identifier.otherPURE UUID: b1a44fc9-c377-4a35-8da8-5a4f30d7972c
dc.identifier.otherdspace: 2299/1670
dc.identifier.urihttp://hdl.handle.net/2299/1670
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/253.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe demonstrate the importance of Ha spectro-polarimetry in constraining the geometry of Herbig Ae/Be stars. We find that discs are common in Herbig Ae and Be stars, although different polarization signatures may imply different modes of accretion.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of the Hot Star Workshop III: the Earliest Stages of Massive Star Birth - ASP Conf Series Vol.267
dc.titleAre all Young Stars Disc Accretorsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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