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Fig. 22


Comparison of the abundances of light neutron-capture elements as derived in HD 122196 to the yields [X/Sr] produced by HEW models. The latter are computed with Ye = 0.45 and varying entropies S (all values listed are given in kB/baryon units). The metallicity ([Fe/H]), and [Ba/Eu] ratio for the star are shown as well.

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