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