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Models and observations of the s process in AGB stars

Lugaro, Maria Anna; Karakas, Amanda; Bisterzo, Sara


Approximately half of the solar abundances of nuclei heavier than iron are created in the deep layers of asymptotic giant branch (AGB) stars via slow neutron captures (the s process). Freshly made heavy elements, such as Zr, Ba, and Pb, are carried to the

CollectionsANU Research Publications
Date published: 2008
Type: Conference paper
Source: 10th Symposium of Nuclei in the Cosmos


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