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Fig. 13


G0 versus ΣSFR derived fromtwo different combinations of luminosities: Hα and 24 μm luminosities (left panel), and FUV and TIR luminosities (right panel). The colour bar corresponds to galactocentric distances in kpc. The coefficients of the linear combinations are taken from Calzetti et al. (2007) and Murphy et al. (2012) for Hα plus 24 μm luminosities and FUV plus TIR luminosities, respectively.

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