Fig. 1.
SFR and s-process yields as a function of metallicity. Upper panel: SFR normalised to SFR at solar RGC at the present time computed with the GCE in the thin disc at RGC = 6, 8, 10 kpc. Middle panel: net yttrium yields as a function of [Fe/H] for a 2 M⊙ AGB star. Bottom panel: net barium yield as a function of [Fe/H] for a 2 M⊙ AGB star (grey: FRUITY yields; red: new MAGN yields).
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