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

Earth, Planets and Space

Table 2. Models.

Name	Species	f _M	P₁ (dyn cm⁻²)	α _f	Grain velocities
A^a	silicate	0.4	3 × 10¹¹	3.3	Yan et al. (2004)
A^a	graphite	0.4	4 × 10¹⁰	3.3	Yan et al. (2004)
B	silicate	0.3	3 × 10¹¹	3.3	Yan et al. (2004)
B	graphite	0.3	4 × 10¹⁰	3.3	Yan et al. (2004)
C	silicate	0.6	3 × 10¹¹	3.3	Yan et al. (2004)
C	graphite	0.6	4 × 10¹⁰	3.3	Yan et al. (2004)
D^a	silicate	0.4	1 × 10¹¹	3.3	Yan et al. (2004)
D^a	graphite	0.4	1.3 × 10¹⁰	3.3	Yan et al. (2004)
E^a	silicate	0.4	9 × 10¹¹	3.3	Yan et al. (2004)
E^a	graphite	0.4	1.2 × 10¹¹	3.3	Yan et al. (2004)
F	silicate	0.4	3 × 10¹¹	2.3	Yan et al. (2004)
F	graphite	0.4	4 × 10¹⁰	2.3	Yan et al. (2004)
G	silicate	0.4	3 × 10¹¹	4.3	Yan et al. (2004)
G	graphite	0.4	4 × 10¹⁰	4.3	Yan et al. (2004)
H	silicate	0.4	3 × 10¹¹	3.3	Eq. (10)
H	graphite	0.4	4 × 10¹⁰	3.3	Eq. (10)