| dc.contributor.author | Napiwotzki, R. | |
| dc.contributor.author | Haas, S. | |
| dc.contributor.author | Schonberner, D. | |
| dc.date.accessioned | 2008-01-27T15:29:45Z | |
| dc.date.available | 2008-01-27T15:29:45Z | |
| dc.date.issued | 1996 | |
| dc.identifier.citation | Napiwotzki , 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.isbn | 1-886733-17-1 | |
| dc.identifier.other | PURE: 146477 | |
| dc.identifier.other | PURE UUID: b0a48a0f-9e24-40ef-9408-ee1f4e63b43b | |
| dc.identifier.other | dspace: 2299/1418 | |
| dc.identifier.uri | http://hdl.handle.net/2299/1418 | |
| dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific | |
| dc.description.abstract | It 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.iso | eng | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.ispartof | In: Hydrogen deficient stars - ASP Conference Series 96 | |
| dc.title | The planetary nebulae of PG 1159 stars - clues to their evolutionary history | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
