University of Hertfordshire

By the same authors

The planetary nebulae of PG 1159 stars - clues to their evolutionary history

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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Original languageEnglish
Title of host publicationIn: Hydrogen deficient stars - ASP Conference Series 96
PublisherAstronomical Society of the Pacific
Pages213-6
ISBN (Print)1-886733-17-1
Publication statusPublished - 1996

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.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific

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