Fig. 2.
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Gas inflow and SFHs in our main models. Top: gas inflow history. Middle top: SFH. Middle bottom: evolution of the total gas mass. Bottom: stellar mass growth. In all panels solid black lines show the model that best reproduces the observed A(Li) evolution of thin-disk stars (SFR_2b), dashed blue lines show the single star formation burst model (SFR_1b), and the dashed red lines show the monotonically decreasing star formation model (SFR_0b).
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