Lugaro, MariaKarakas, AmandaStancliffe, RichardRijs, Carlos2015-12-13November 19780735410961http://hdl.handle.net/1885/71574We have performed calculations for the slow neutron capture process (the s process) in stellar models of mass from 0.9 M⊙ to 6 M ⊙ at a metallicity of [Fe/H]=-2.3. The models were computed with two different stellar evolution codes and our results comKeywords: Abundances; Nucleosynthesis; Stars: Abundances; Stars: AGB and Post-AGB201210.1063/1.47633822016-02-24