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Earth, Planets and Space
Fig. 4. | Earth, Planets and Space

Fig. 4.

From: Evolution of dust grain size distribution by shattering in the interstellar medium: Robustness and uncertainty

Fig. 4.

Same as Fig. 2 but for Models A, F, and G, in order to investigate the effect of αf (power index of the grain size distribution of shattered fragments). The solid, dashed, and dot-dashed lines show the results at t = 10 Myr for Models A, D, and E (αf = 3.3, 2.3, and 4.3), respectively. The dotted line presents the initial grain size distribution before shattering.

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