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Fig. 12


[C ii] and [O i]-to-CO ratios versus 70 μm/100 μm. The horizontal orange band indicates the average ratio [C ii]/CO(1–0) of 2000–6000 observed in star-forming regions of the Galaxy and galaxies (Stacey et al. 1991). For the [C ii]/CO(3–2) horizontal band, a ratio R31 = 0.6 is considered. The blue circles correspond to the model predictions for Haro 11.

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