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Fig. 2.

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Mass-weighted projections of the gas density (top two left panels), temperature (top two middle panels), dust-to-metal mass ratio (top two right panels), and dust-to-gas mass ratio (bottom two left panels), small grain fraction (bottom two middle panels), and carbonaceous grain fraction (bottom two right panels), viewed edge-on (top panel with a depth of 30 kpc) or face-on (bottom panel with a depth of 600 pc) for the high resolution version of G10LG galaxy with the fiducial physics at t = 400 Myr. In black are shown isocontours of density with n = 1 H cm−3.

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