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Post-AGB Candidates
Published online by Cambridge University Press: 07 August 2017
Abstract
A review is given of the properties of post-AGB stars. Methods to find candidate post-AGB stars are briefly discussed, along with some results and selection effects involved. Their photospheric parameters (Teff, log g, abundances), energy distributions and binarity are also discussed. Evidence for mass loss, both past and present, is reviewed.
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- IV. Planetary Nebulae Connection: Evolution from the AGB
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- Copyright © Kluwer 1993
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