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dc.contributor.authorGledhill, T.
dc.contributor.authorYates, J.A.
dc.contributor.authorChrysostomou, A.
dc.date.accessioned2008-01-30T10:36:15Z
dc.date.available2008-01-30T10:36:15Z
dc.date.issued2000
dc.identifier.citationGledhill , T , Yates , J A & Chrysostomou , A 2000 , Imaging Linear Polarimetry of Proto-planetary Nebulae: the Origins of Asymmetry . in In: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199 . Astronomical Society of the Pacific , pp. 151-4 .
dc.identifier.isbn1-58381-026-9
dc.identifier.otherPURE: 180481
dc.identifier.otherPURE UUID: 1f3a0804-061c-4b75-8dc6-99fba7c1b150
dc.identifier.otherdspace: 2299/1439
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779796
dc.identifier.urihttp://hdl.handle.net/2299/1439
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/195-221.html--Copyright Astronomical Society of the Pacific
dc.description.abstractIt now seems likely that asymmetries in the circumstellar envelope (CSE) of intermediate mass stars develop during the latter stages of mass outflow as a star approaches the tip of the AGB. These asymmetries in the CSE must in some way give rise to the range of morphologies pbserved in planetary nebulae (PN) and their antecedants proto-planetary nebulae (PPN). We use imaging linear polarimetry to trace scattering in the CSEs and to reveal a morphologically diverse sample of PPN.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199
dc.rightsOpen
dc.titleImaging Linear Polarimetry of Proto-planetary Nebulae: the Origins of Asymmetryen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2000
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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