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Fig. 9.
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Dust-to-metal ratio (DTM, top left), dust-to-gas ratio (DTG, top right), fraction of small grains fS (bottom left), and fraction of carbonaceous grains fC (bottom right) as a function of density n and temperature T for the G10LG galaxy at time t = 400 Myr. Black contours are for the mass distribution of gas.
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