Fig. 11.
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Dependencies of the duration of the obscured star-formation time (tobscured). Left: Duration of the obscured star-formation time as a function of the morphological type of galaxies from the HyperLEDA database (Paturel et al. 2003a,b; Makarov et al. 2014). The color bar shows the gas-phase metallicity measured with MUSE. Right: Duration of the obscured star-formation phase (bottom) as a function of gas-phase metallicity. The color bar shows the evolution of the SFR surface density.
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