Table 1
Summary of the CSM properties we adopted as initial conditions for our model grid.
 |
RCSM (1014 cm) | MCSM(M⊙) | Rphot [1014 cm] |
|---|---|---|---|
| 0.001 | 2 | 8.62(–3) | 1.39 |
| 0.001 | 6 | 1.07(–2) | 2.56 |
| 0.001 | 10 | 1.35(–2) | 3.42 |
| 0.01 | 2 | 2.40(–2) | 1.68 |
| 0.01 | 6 | 4.43(–2) | 4.14 |
| 0.01 | 10 | 7.19(–2) | 7.32 |
| 0.1 | 2 | 1.75(–1) | 1.80 |
| 0.1 | 6 | 3.72(–1) | 4.70 |
| 0.1 | 10 | 6.50(–1) | 8.48 |
Notes. The columns give the correspondence between the CSM density (i.e., Ṁ) and the extent (RCSM) on the one hand, and the CSM mass and the radius of the electron-scattering photosphere initially on the other hand. For the latter, an ionized H-rich CSM was assumed (i.e., κ = 0.34 cm2 g−1). All simulations presented here were based on a ZAMS star of 15 M⊙ evolved at solar metallicity. See Sect. 2 for a discussion.
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