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Fig. 10


Metallicities and effective yields as a function of gas fraction for the galaxies in our sample at z ~ 3, with the same symbols as in the previous figures. In both panels the Erb (2008) models for various inflows fi, outflows fo rates (relative to the SFR) are shown. The dotted black line is the closed-box model (fi = fo = 0). In the bottom panel (lower-right corner), the inflows and outflows rates in units of the SFR are shown for every model (with different color-coding).

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