Synthetic post-AGB evolution

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[1] Frankowski, A.
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Frankowski, A. (frankowski@ncac.torun.pl) | 1600年 / EDP Sciences卷 / 406期
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Mathematical models - Numerical methods - Opacity - Parameter estimation - Solar system - Stress analysis;
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摘要
A synthetic method for tracing the evolution of the post-AGB stars, based on existing numerical calculations was presented. It was used to obtain post-AGB evolutionary tracks of solar and SMC metallicity, with possible extension to higher core masses. The model allows fast computing of extensive grids of models for post-AGB objects of different parameters.
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