Fig. 6.From: Evolution of dust grain size distribution by shattering in the interstellar medium: Robustness and uncertaintySame as Fig. 2 but for Model H with various ac. The solid, and dashed lines show the results for ac = 10− and 10−6 cm, respectively. The dotted line presents the initial grain size distribution before shattering, and the dot-dashed line shows the results for Model A as a reference.Back to article page