Element Enhancements along the Entire Asymptotic Giant Branch Phase
The results of a study of the asymptotic giant branch (AGB) phase of stellar evolution are presented. Abundances have been determined for Fe, C, O, the light s-process elements, Y and Zr, the heavy s-process elements, La and Nd, and the r-process element,
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|Source:||Astrophysical Journal, The|
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