Table 1
Initial conditions.
| Case | MZAMS (M⊙) | Rw (pc) | Re (pc) | Rsn (pc) | Msn (M⊙) | Esn (erg) | 56Ni mass (M⊙) | Min. Res. (pc) | Max. Res. (pc) |
|---|---|---|---|---|---|---|---|---|---|
| S200 | 60 | 0.04 | 0.06 | 0.04 | 10 | 1051 | – | 1.5 × 10−2 | 3.9 × 10−3 |
| S200−Test | 60 | 0.04 | 0.06 | 0.04 | 10 | 1051 | – | 1.5 × 10−2 | 7.8 × 10−3 |
| B200 | 60 | 0.04 | 0.06 | 0.04 | 10 | 1051 | – | 7.8 × 10−3 | 1.9 × 10−3 |
| B200−Test | 60 | 0.04 | 0.06 | 0.04 | 10 | 1051 | – | 7.8 × 10−3 | 7.8 × 10−3 |
| B12−10 | 60 | 0.008 | 0.0012 | 0.0015 | 10 | 1051 | – | 1.9 × 10−4 | 4.8 × 10−5 |
| B12−10–Test | 60 | 0.008 | 0.0012 | 0.0015 | 10 | 1051 | – | 1.9 × 10−4 | 9.7 × 10−5 |
| B12−56Ni | 60 | 0.008 | 0.0012 | 0.0015 | 10 | 1051 | 0.032 | 1.9 × 10−4 | 4.8 × 10−5 |
| B12−15 | 45 | 0.008 | 0.0012 | 0.0015 | 15 | 5 × 1051 | 0.9 | 1.9 × 10−4 | 4.8 × 10−5 |
| B12−20 | 50 | 0.008 | 0.0012 | 0.0015 | 20 | 5 × 1051 | 2.5 | 1.9 × 10−4 | 4.8 × 10−5 |
Notes. For each case, we assume for the stellar wind a mass-loss rate of Ṁw = 10−3 M⊙ yr−1 and a terminal velocity of υ∞ = 250 km s−1. The eruption mass and energy are 25 M⊙ and 1050 erg, respectively, with a dust mass of 0.25 M⊙. From left to right, the table presents the ZAMS mass of the progenitor, the insertion radius of the stellar wind, eruption, and SNR, the mass of 56Ni, and both the minimum and maximum resolutions for each case.
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