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Fig. 5.

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⟨Log(SFR/M*)⟩ as a function of Log(M*/M) for ringed galaxies (solid red lines) and for galaxies in the control sample (long-dash black lines). Left panel: galaxies with an inner ring (dashed line magenta) and galaxies with other types of rings (two-dash blue line). Right panel: non-barred ringed galaxies (dashed cyan line) and barred ringed galaxies (two-dash green line).

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