MH2 vs. LB for a) spiral galaxies (T ≥ 1) and b) elliptical (circles) and S0 galaxies (triangles). LFIR vs. LB for c) spiral galaxies (T ≥ 1) and d) elliptical (circles) and S0 galaxies (triangles). The full green line corresponds to the bisector fit found for HCG galaxies (fit parameters are given in Table 4), while the blue dashed-dotted line corresponds to the bisector fit found for the AMIGA isolated galaxies. Both fits are done for the entire range of morphological types. The dashed black lines are offset by the standard deviation of the correlation for the isolated galaxies, which is ± 0.35 for the MH2 and ± 0.4 for LFIR. Black symbols denote detections and red symbols upper limits.
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