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Fig. 8


Histogram of the atomic neutral gas thermal pressures and surface temperatures obtained by applying the PDR modeling to the galaxies belonging to different galaxy samples. The local SFGs and starbursts belonging to the SHINING sample, and the samples from Malhotra et al. (2001) and Negishi et al. (2001) are shown in gray; the subsample of galaxies classified as LINERs, Sy1 and Sy2, are shown in pink; and the low-metallicity dwarf galaxies from Cormier et al. (2015) are shown in green. The ranges of ISM parameters obtained by modeling the LBAs and the ZEUS samples at z ~ 1−2 are shown in yellow and light blue, respectively.

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