Fig. E.6.
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SF efficiency as a function of the velocity dispersion of the regions (σv, regions) across the merger sequence. From left to right and top to bottom, the merger stages are: isolated galaxies (blue), galaxy pairs (red), early-stage mergers (orange), mid-stage mergers (magenta) and late-stage mergers (black). The Spearman’s rank correlation coefficients (ρs) are indicated. The bottom right panel shows the mean values of σv, regions and log10SFEregions, with error bars representing the mean absolute deviation for each merger stage.
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