Fig. 12
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Abundance ratios of [Sr/Fe] versus [Fe/H]. The red dots are the abundances of the GSE stars in our sample; the colour-coded area shows the results of the stochastic model. The colour coding is described in the bar as the number density of long-living stars in log-scale. The black line shows the most probable value of the model in [Sr/Fe] at each bin in [Fe/H].
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