Table B.1
Properties of DARWIN models with outflows driven by photon scattering on Fe-free silicate grains.
model | Ṁ | uext | fSi | fMg | agr |
---|---|---|---|---|---|
name | [M⊙/yr] | [km/s] | [μm] | ||
An115u3 | 1 ⋅ 10−7 | 2 | 0.17 | 0.32 | 0.47 |
An315u3 | 3 ⋅ 10−7 | 5 | 0.20 | 0.37 | 0.34 |
An114u3 | 4 ⋅ 10−7 | 7 | 0.27 | 0.50 | 0.25 |
An314u3 | 4 ⋅ 10−7 | 7 | 0.38 | 0.71 | 0.20 |
An115u4 | 3 ⋅ 10−7 | 3 | 0.17 | 0.32 | 0.47 |
An315u4 | 5 ⋅ 10−7 | 6 | 0.20 | 0.37 | 0.34 |
An114u4 | 6 ⋅ 10−7 | 9 | 0.27 | 0.50 | 0.25 |
An314u4 | 5 ⋅ 10−7 | 8 | 0.37 | 0.69 | 0.20 |
Bn316u3 | 3 ⋅ 10−7 | 2 | 0.13 | 0.24 | 0.64 |
Bn115u3 | 5 ⋅ 10−7 | 5 | 0.14 | 0.26 | 0.44 |
Bn315u3 | 7 ⋅ 10−7 | 7 | 0.17 | 0.32 | 0.33 |
Bn114u3 | 8 ⋅ 10−7 | 8 | 0.24 | 0.45 | 0.24 |
Bn314u3 | 8 ⋅ 10−7 | 8 | 0.35 | 0.65 | 0.19 |
Bn316u4 | 3 ⋅ 10−7 | 2 | 0.13 | 0.24 | 0.64 |
Bn115u4 | 5 ⋅ 10−7 | 4 | 0.13 | 0.24 | 0.43 |
Bn315u4 | 7 ⋅ 10−7 | 6 | 0.17 | 0.32 | 0.33 |
Bn114u4 | 8 ⋅ 10−7 | 8 | 0.24 | 0.45 | 0.24 |
Bn314u4 | 8 ⋅ 10−7 | 8 | 0.34 | 0.64 | 0.19 |
M2n115u6 | 1 ⋅ 10−6 | 5 | 0.19 | 0.36 | 0.49 |
M2n315u6 | 2 ⋅ 10−6 | 12 | 0.23 | 0.43 | 0.36 |
M2n114u6 | 2 ⋅ 10−6 | 14 | 0.32 | 0.60 | 0.27 |
Notes. The capital letters in the model name denote different combinations of stellar parameters (see Sect. 3), the letter n followed by a 3-digit number stands for the seed particle abundance (i.e., n316 for nd ∕nH = 3 ⋅ 10−16, n115 for nd ∕nH = 1 ⋅ 10−15, etc.) and the letter u followed by a number represents the velocity amplitude at the inner boundary ΔuP (km/s). The resulting wind and dust properties listed here are temporal means of the mass-loss rate Ṁ, the wind velocity uext, the fraction of Si condensed into grains fSi, the fraction of Mg condensed into grains fMg, and the grain radius agr. The values for models of series A and B listed here are taken from Paper I (Höfner et al. 2016).
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