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Fig. 5

image

Specific star formation rate, log (SFR/M), and Dn(4000) (upper and lower panels) as a function of stellar mass bins for unbarred, weak and strong-barred spiral galaxies that belong to the major peaks of the star formation and stellar population distributions (see Fig. 3) (solid, dotted, and dashed lines, respectively).

This figure is made of several images, please see below:

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