Fig. 7.
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Plots comparing difference in SFR (log(ΔSFR) = logSFRpost − merger − logSFRnon − interacting) of post-merger with respect to non-interacting control dwarfs. Left panel: Histogram distribution of SFR offset for the entire galaxy and its central and outer regions. Right panel: Histogram distribution of SFR offsets for visually identified dwarf galaxy sample and its central and outer regions.
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