Metallicity dependence of the CO-to-H2 and the [CI]-to-H2 conversion factors in galaxies

Open Access

Fig. 8

Logarithmic grid maps as in shown in Figs. 3 and 4, but colored with respect to the logarithmic f_DARK CO-dark gas fraction. The upper row shows results for the m = 5 and σ_PDF = 0.4 distribution, and the bottom row shows results for the m = 15 and σ_PDF = 0.4 distribution.

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