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Heavy Element Nucleosynthesis in the Brightest Galactic Asymptotic Giant Branch stars

ASTROPHYSICAL JOURNAL, no. 1 (2012)

引用：88|浏览26

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academic.microsoft.com arxiv.org

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nuclear reactions nucleosynthesis abundancesstars: abundancesstars: AGB and post-AGB

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We present updated calculations of stellar evolutionary sequences and detailed nucleosynthesis predictions for the brightest asymptotic giant branch (AGB) stars in the Galaxy with masses between 5M(circle dot) and 9M(circle dot), with an initial metallicity of Z = 0.02 ([Fe/H] = 0.14). In our previous studies we used the Vassiliadis & Woo...更多

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