The s-process in asymptotic giant branch stars of low metallicity and the composition of carbon-enhanced metal-poor stars
We present models for the slow neutron-capture process (s-process) in asymptotic giant branch stars of metallicity [Fe/H] = -2.3 and masses 0.9-6 M·. We encountered different regimes of neutron-capture nucleosynthesis listed here increasing in importance
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|Source:||Astrophysical Journal, The|
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