Fig. 7.
L[C II/SFR ratio as a function of pressure, colour-coded by SFR. We present the mean value of SFR for each bin for the galaxies in the three simulations assuming they represent the same population. Pressure is anti-correlated with the L[C II/SFR ratio, in agreement with the result presented by Popping et al. (2019). We have confirmed that the trends do not depend on the specific simulation used.
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