From red giant to planetary nebula: Dust, asymmetry, and polarization

Joni Jayne Johnson, Terry Jay Jones

Research output: Contribution to journalArticlepeer-review

62 Scopus citations

Abstract

The polarization characteristics of stars in the stages of evolution from red giant to planetary nebula are investigated. Polarization is found to be a characteristic of the majority of these stars. The maximum observed polarization increases with age as the star evolves up the asymptotic giant branch (AGB) to the protoplanetary nebula phase, where the polarization reaches a maximum. The polarization then decreases as the star further evolves into a planetary nebula. Our results indicate that aspherical mass loss is likely to be a continual feature of the late stages of stellar evolution, maintaining a clear continuity throughout the life of a star from the moment it first develops a measurable dust shell. The aspherical morphology seen in planetary nebulae has its origin in an intrinsic property of the star that is present at least as early as its arrival at the base of the AGB.

Original languageEnglish (US)
Pages (from-to)1735-1751
Number of pages17
JournalAstronomical Journal
Volume101
Issue number5
DOIs
StatePublished - May 1991

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