Table 1.
Summary of interaction configurations simulated with HERACLES together with properties of the CDS and the model radiation.
| Model | Explosion |
CSM: Wind |
CDS |
Light curve |
||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Ekin | Mej | M(56Ni) | Ṁ | V∞ | V(CDS) | M(CDS) | tpeak | Lpeak | ∫Ldt | |
| [1049 erg] | [M⊙] | [M⊙] | [M⊙ yr−1] | [1000 km s−1] | [1000 km s−1] | [M⊙] | [d] | [1042 erg s−1] | [1049 erg] | |
| W1 | 7.5 | 1.49 | 0.08 | 0.001 | 1.0 | 6.37 | 0.0051 | 29.8 | 1.58 | 0.45 |
| W2 | 7.5 | 1.49 | 0.08 | 0.01 | 1.0 | 4.99 | 0.0201 | 28.8 | 1.73 | 0.53 |
| W3 | 7.5 | 1.49 | 0.08 | 0.1 | 1.0 | 3.57 | 0.0974 | 1.1 | 3.43 | 0.78 |
| W4 | 75.0 | 1.49 | 0.08 | 0.001 | 1.0 | 18.98 | 0.0086 | 11.7 | 4.45 | 0.96 |
| W5 | 75.0 | 1.49 | 0.08 | 0.01 | 1.0 | 13.65 | 0.0424 | 0.3 | 23.73 | 2.59 |
| W6 | 75.0 | 1.49 | 0.08 | 0.1 | 1.0 | 8.83 | 0.2523 | 1.1 | 91.73 | 8.90 |
| W7 | 7.5 | 0.15 | 0.008 | 0.001 | 1.0 | 13.71 | 0.0043 | 0.2 | 4.24 | 0.31 |
| W8 | 7.5 | 0.15 | 0.008 | 0.01 | 1.0 | 8.84 | 0.0254 | 0.3 | 12.26 | 0.95 |
| W9 | 7.5 | 0.15 | 0.008 | 0.1 | 1.0 | 5.59 | 0.1168 | 1.0 | 30.77 | 2.52 |
| Model | Explosion |
CSM: Ejecta |
CDS |
Light curve |
||||||
| Ekin | Mej | M(56Ni) | Ekin | Mej | V(CDS) | M(CDS) | tpeak | Lpeak | ∫Ldt | |
| [1049 erg] | [M⊙] | [M⊙] | [1049 erg] | [M⊙] | [1000 km s−1] | [M⊙] | [d] | [1042 erg s−1] | [1049 erg] | |
| E1 | 7.5 | 1.49 | 0.08 | 0.01 | 1.0 | 1.67 | 1.4761 | 9.3 | 39.2 | 2.48 |
| E2 | 7.5 | 1.49 | 0.08 | 1.0 | 1.0 | 1.96 | 1.3637 | 10.8 | 13.3 | 1.45 |
| E3 | 75.0 | 1.49 | 0.08 | 0.01 | 1.0 | 4.56 | 1.8138 | 8.9 | 460.6 | 29.1 |
| E4 | 75.0 | 1.49 | 0.08 | 1.0 | 1.0 | 4.91 | 1.7519 | 9.1 | 323.8 | 23.1 |
| E5 | 7.5 | 0.15 | 0.008 | 0.01 | 1.0 | 1.37 | 1.0127 | 11.4 | 41.8 | 5.7 |
| E6 | 7.5 | 0.15 | 0.008 | 1.0 | 1.0 | 2.08 | 0.8853 | 10.7 | 33.3 | 4.2 |
Notes. The properties of the CDS are given at 40 d after the onset of the interaction. At this time, most of the CSM has been swept-up so the CDS properties are no longer changing. For the time-integrated bolometric luminosity, the integral covers from the time of the first record of radiation at the outer boundary until the end of the simulations at 50 d. This covers the main part of the high-brightness phase.
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