Table 2
Comparison of this study to different forward shock dust destruction studies after 10 kyr.
| Paper | ISM inhomogeneities | n | Resolution | gg | GSD | Dust destr. for n ≈ 1 cm−3 at 10 kyr |
|---|---|---|---|---|---|---|
| this work | turbulence | 1–100 cm−3 | 0.022–0.044 pc | yes | MRN | 0.85–1.53 M⊙ (27.3–56.8%) |
| [1] | clumps | 0.3–10 cm−3 | 0.19–0.5 pc | no | MRN | 0.67–1.17 M⊙ (32–39%) |
| [2] | turbulence | 0.7 cm−3 | 0.5 pc | yes | MRN | 2.8 M⊙ |
| [3] | weakly inhomogeneous | 0.1–1 cm−3 | 0.5 pc | yes | MRN | 6.95 M⊙ |
| [4] | wind-driven bubble | 1, 1000 cm−3 | 0.11–0.21 pc | no | log-normal | 0.40 M⊙ |
Notes. [1] Dedikov & Vasiliev (2025), [2] Kirchschlager et al. (2024a), [3] Kirchschlager et al. (2022), [4] Martínez-González et al. (2019). Compared are the ISM inhomogeneity model, the average ISM density ( $n$ ), the resolution, whether grain-grain collisions are considered or not (gg), the initial grain-size distribution (GSD), and the destroyed dust mass (and rate) after the first 10 kyr of SNR evolution for n ≈ 1 cm−3 cases.
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