Fig. 6
MH2 vs. LFIR for late-type (T ≥ 1, squares) and early-type (E+S0, crosses) galaxies. The green line corresponds to the bisector fit found for HCGs galaxies, while the blue dashed-dotted line corresponds to the bisector fit found for the AMIGA isolated galaxies from Lisenfeld et al. (2011). The fits are detailed in Table 4. The dotted black lines correspond to the LFIR/MH2 ratios 1 (left), 10 (middle), and 100 (right) L⊙/M⊙. Black symbols denote detections and red symbols upper limits.
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