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Table 5.
SN II dust yields.
| Individual star mass, m⋆ | Dust yield,  |
|---|---|
| 8.5 M⊙ | 0 M⊙ × δSN |
| 9 M⊙ | 0.17 M⊙ × δSN |
| 12 M⊙ | 0.2 M⊙ × δSN |
| 15 M⊙ | 0.5 M⊙ × δSN |
| 20 M⊙ | 0.5 M⊙ × δSN |
| 22 M⊙ | 0.8 M⊙ × δSN |
| 25 M⊙ | 1.0 M⊙ × δSN |
| 30 M⊙ | 1.0 M⊙ × δSN |
| 35 M⊙ | 0.6 M⊙ × δSN |
| 40 M⊙ | 0.4 M⊙ × δSN |
Notes. These values are the Todini & Ferrara (2001) yields, compiled by Rowlands et al. (2014). They are multiplied by the tuning parameter δSN, used by De Vis et al. (2017a).
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