Barium stars as tracers of s-process nucleosynthesis in AGB stars - II. Using machine learning techniques on 169 stars

Open Access

Fig. 11

Same figure format as in Fig. 4. There are no classifications with a GoF above 50% for this star due to the strong increase in the elemental abundances of the first s-process peak and the strong decrease in the elemental abundances of the second s-process peak.

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