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Fig. 4

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Contribution of each dust component to the average extinction curve of the MW-like galaxy simulation at various times (t = 0.1, 0.5, 3.0, and 10.0 Gyr). The black thick line is the total average extinction curve, while the orange solid, green dashed, blue dotted, and light blue dash-dotted thin lines represent the contributions of silicate, graphite, PAH0, and PAH+, respectively. At t = 0.1 Gyr, the extinction curve is dominated by silicate grains across all wavelengths. However, at later times, carbonaceous grains become the dominant contributors to extinction at wavelengths longer than 2000 Å.

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