The impact of updated Zr neutron-capture cross sections and new asymptotic giant branch models on our understanding of the S process and the origin of stardust
Date
2014
Authors
Lugaro, Maria
Tagliente, G
Karakas, Amanda
Milazzo, P M
Kappeler, F
Davis, Andrew M
Savina, Michael R.
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IOP Publishing
Abstract
We present model predictions for the Zr isotopic ratios produced by slow neutron captures in C-rich asymptotic giant branch (AGB) stars of masses 1.25-4 M⊙ and metallicities Z = 0.01-0.03, and compare them to data from single meteoritic stardust silicon
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Astrophysical Journal, The
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Journal article
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2037-12-31
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