Synthetic post-AGB evolution
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Rabiańska 8, 87–100 Toruń, Poland
Corresponding author: firstname.lastname@example.org
Accepted: 13 May 2003
A synthetic method for tracing the evolution of the post-AGB stars, based on existing numerical calculations, 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.
Key words: stars: evolution / stars: AGB and post-AGB
© ESO, 2003