Dust and gas modeling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D

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Fig. 11

Probability density distribution function for the molecular fraction f_mol (see Sect. 3.2). All the distributions feature a major peak around f_mol ~ 0 (fully atomic gas) and a less significant peak around f_mol ~ 1 (fully molecular gas). The displayed curves are normalized so that they subtend an area equal to unity.

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