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This article has an erratum: [https://doi.org/10.1051/0004-6361/201322104e]


Fig. 8

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Distribution of corrected Hubble residuals per ΣHα group (top, as in Fig. 6) and per mode (bottom) for the full sample. In the lower panel, the open-red and the filled-gray histograms represent the corrected Hubble residual distributions of M1 and M2, respectively. By definition of the modes, the red histogram corresponds to the stack of the blue distribution with the open histogram above (see the top-panel), while the filled-gray histogram corresponds to the part of the open histogram below . Colored solid lines (red for M1 and black for M2) show the best fit by a normal distribution (with 3σ clipping). Fit parameters are quoted beside each Gaussian.

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