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dc.contributor.authorNapiwotzki, R.
dc.contributor.authorHaas, S.
dc.contributor.authorSchonberner, D.
dc.date.accessioned2008-01-27T15:29:45Z
dc.date.available2008-01-27T15:29:45Z
dc.date.issued1996
dc.identifier.citationNapiwotzki , R , Haas , S & Schonberner , D 1996 , The planetary nebulae of PG 1159 stars - clues to their evolutionary history . in In: Hydrogen deficient stars - ASP Conference Series 96 . Astronomical Society of the Pacific , pp. 213-6 .
dc.identifier.isbn1-886733-17-1
dc.identifier.otherPURE: 146477
dc.identifier.otherPURE UUID: b0a48a0f-9e24-40ef-9408-ee1f4e63b43b
dc.identifier.otherdspace: 2299/1418
dc.identifier.urihttp://hdl.handle.net/2299/1418
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific
dc.description.abstractIt is shown that many planetary nebulae (PN) surrounding PG 1159 stars display a bipolar morphology. The frequency of these nebulae is higher than observed in other PN samples. Implications for the evolutionary history of the PG 1159 stars are discussed. Judged from our present day knowledge of PN formation it is likely that many PG 1159 stars are the result of some sort of binary evolution.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Hydrogen deficient stars - ASP Conference Series 96
dc.rightsOpen
dc.titleThe planetary nebulae of PG 1159 stars - clues to their evolutionary historyen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1996
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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