Carbon- and s-Process-Rich Post-AGB Stars: Theoretical Interpretations

The study of post-AGB stars gives important informations on the s-process inside AGB stars, as the s-enrichment of post-AGB stars is due to an intrinsic process. A sample of thirteen C-and s-rich post-AGB stars were analyzed with AGB nucleosynthetic models at different masses, metallicities and s-pr...

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Hauptverfasser:	Gallino, R, Bisterzo, S, Husti, L
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Sprache:	eng
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creator	Gallino, R Bisterzo, S Husti, L
description	The study of post-AGB stars gives important informations on the s-process inside AGB stars, as the s-enrichment of post-AGB stars is due to an intrinsic process. A sample of thirteen C-and s-rich post-AGB stars were analyzed with AGB nucleosynthetic models at different masses, metallicities and s-process efficiencies. We present and discuss the theoretical fits obtained for 3 selected stars of our sample. A summary of the results obtained by comparing spectroscopic abundances and AGB theoretical models for all the considered stars is reported.
doi_str_mv	10.1063/1.2916954
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identifier	ISSN: 0094-243X
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title	Carbon- and s-Process-Rich Post-AGB Stars: Theoretical Interpretations
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