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Earth, Planets and Space
Fig. 3. | Earth, Planets and Space

Fig. 3.

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

Fig. 3.

Same as Fig. 2 but for Models A, D, and E. The thick solid, dashed, and dot-dashed lines show the results at t = 10 Myr for Models A, D, and E (fiducial, hard, and soft grains), respectively, while the thin lines adopt the treatment of fragments by KT10 (the same line species shows the same model). The dotted line presents the initial grain size distribution before shattering. Two grain species, (a) silicate and (b) carbonaceous dust, are shown.

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