Fig. 13.

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Spatial distribution of star formation rate averaged over different timescales. Left three panels: Surface density distributions of star formation rate averaged over the last 107, 108 and 109 yr (i.e., the birth mass of stars younger than the age limits divided by the age limits), respectively. The black contours overplotted in the left three panels correspond to 50% of the maximum ΣSFR. Rightmost panel: Surface density distribution of stellar mass.
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