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Evolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars. II. s-process nucleosynthesis during the core He flash

Campbell, Simon; Lugaro, Maria; Karakas, Amanda

Description

Methods. We perform post-process nucleosynthesis calculations on a one-dimensional stellar evolution calculation of a star with mass 1 M· and a metallicity of [Fe/H] =-6.5 that suffers a proton ingestion episode. Our network includes 320 nuclear species

CollectionsANU Research Publications
Date published: 2010
Type: Journal article
URI: http://hdl.handle.net/1885/37433
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201015428

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