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Fig. 3

image

Comparison between CALIFA MS (green dashed lines), control sample (blue dash-dotted lines), and interacting sample (red solid lines). Top: stellar mass distributions for these samples. Stellar masses for each galaxy is taken from Walcher et al. (2014). Vertical lines represent the stellar mass range where CALIFA MS is considered to be representative of the nearby galaxy population. Bottom: morphological distributions of these three samples.

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