Models and observations of the s process in AGB stars
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
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|Source:||10th Symposium of Nuclei in the Cosmos|
|01_Lugaro_Models_and_observations_of_the_2008.pdf||265.97 kB||Adobe PDF||Request a copy|
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