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Synthetic Post-AGB Evolution

Published online by Cambridge University Press:  26 May 2016

Adam Frankowski
Adam Frankowski*
Affiliation:
N. Copernicus Astronomical Center, ul. Rabiańska 8, 87-100 Toruń, Poland

Abstract

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A synthetic method for tracing the evolution of the post-AGB stars is presented. The main advantage of this procedure, based on the published numerical evolutionary sequences, is that it is simple, fast, and allows to treat post-AGB objects of arbitrary mass.

Type
Part III: Planetary Nebulae in the Scheme of Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 109 - 110
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Blöcker, T. 1995, A&A, 299, 755 Google Scholar
Paczyński, B. 1971, AcA, 21, 41 Google Scholar
Schönberner, D. 1981, A&A, 103, 119 Google Scholar
Schönberner, D. 1983, ApJ, 272, 708 Google Scholar
Vassiliadis, E. & Wood, P.R. 1993, ApJ, 413, 641 CrossRefGoogle Scholar
Vassiliadis, E. & Wood, P.R. 1994, ApJS, 92, 125 Google Scholar