Image Details
Caption: Figure 5.
Torino AGB model predictions with various 13C-pocket internal structures in the D1.5 case for a 2 M☉, 0.5 Z☉ AGB star are shown in the three-isotope plots of δ(92Zr/94Zr) vs. δ(96Zr/94Zr), δ(88Sr/86Sr) vs. δ(84Sr/86Sr), and δ(138Ba/136Ba) vs. δ(135Ba/136Ba).
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