Fig. 17.
Neutron-capture abundances observed in HD 94028 are compared to the predictions of the main r-process following Wanajo (2007, hot and cold models, blue lines) in the top panel; the solar abundance pattern (green line) in the middle panel; and the predictions of the combined s, modified r, and i-processes as computed by Roederer et al. (2016, their Figs. 6 and 7; red lines) in the bottom panel.
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