Measuring the physical imprints of gas flows in galaxies - I. Accretion rate histories

Open Access

Fig. 3.

Set of ChEH (top) and SFH (bottom) corresponding to the averaged histories of all galaxies in our sample. In the top panel, the solid line corresponds to out measured ChEH and the dashed line to the predicted enrichment history in the absence of dilution from pristine gas accretion.

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