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Fig. 7


LBAs on the ISRF (expressed in G0 units) – atomic gas density nH plane as inferred from the PDR modeling (following Kaufman et al. 1999). We also plot the results of the same modeling for the subsample of SHINING galaxies that have [OI],[CII], and FIR observations (Graciá Carpio et al. 2011; Herrera-Camus et al., in prep.), some resolved regions inside M82 (Contursi et al. 2013), the central regions of local SFGs observed with ISO-LWS (Malhotra et al. 2001; Negishi et al. 2001), the sample of local dwarfs from Cormier et al. (2015), and a sample of z~1−2 SFGs observed with ZEUS (Brisbin et al. 2015).

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