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Fig. 19


The molecular gas mass vs. LB for different sample of interacting galaxies: Galaxies of type T = 3–5 from the sample of Casasola et al. (2004) and a sample of weakly (WPER) and strongly (SPER) perturbed galaxies from Perea et al. (1997). We adapted both the molecular gas masses and LB to our definition. The full line is the regression fit obtained for the AMIGA T = 3–5 sample from Table 7.

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