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Post-AGB Candidates

Published online by Cambridge University Press:  07 August 2017

L.B.F.M. Waters  and
K.C. Sahu
L.B.F.M. Waters
Affiliation:
Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam SRON Laboratory for Space Research Groningen, P.O. Box 800, 9700 AV Groningen
K.C. Sahu
Affiliation:
Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen

Abstract

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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.

Keywords

post-AGB starsmass lossevolutionbinarity
Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 271 - 278
Copyright
Copyright © Kluwer 1993 

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