Fig. 5.

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Distribution of central SFR indicators for galaxies with strong arms and the control sample with weak arms. Panels a–d: show the result of sSFRfiber, C(sSFR), Dn(4000), and HδA, respectively. The distributions for strong-armed galaxies are marked in blue, and the same for the control weak-armed sample are marked in gray. The mean difference between the two distributions and p values from the Kolmogorov–Smirnov test are presented at the top of each panel.
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