Table 1.
Summary of properties for the progenitor, the ejecta, the magnetar, as well as results at bolometric maximum obtained with the CMFGEN simulations.
| Model | 56Ni | Mej | Ekin | Epm | Ppm | Bpm | V0 | dV | tpm | tpeak | Lpeak |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (M⊙) | (erg) | (erg) | (ms) | (G) | (km s−1) | (km s−1) | (d) | (d) | (erg s−1) | |
| 5p11Bx2th | 0.19 | 3.63 | 2.49(51) | 0.4(51) | 7.0 | 3.5(14) | 6000 | 3000 | 19.1 | 26.0 | 4.83(43) |
| 5p11Bx2 | 0.19 | 3.63 | 2.49(51) | 0.4(51) | 7.0 | 3.5(14) | 6000 | 3000 | 19.1 | 26.7 | 4.86(43) |
| r0e2 | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 3.5(14) | 5700 | 2850 | 19.1 | 31.7 | 3.75(43) |
| r0e2n | 0.13 | 9.69 | 4.12(51) | ... | ... | ... | ... | ... | ... | 44.4 | 2.25(42) |
| r0e2 | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 3.5(14) | 5700 | 2850 | 19.1 | 31.7 | 3.75(43) |
| r0e2s | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 3.5(14) | 1425 | 713 | 19.1 | 51.7 | 2.81(43) |
| r0e1 | 0.09 | 9.52 | 1.14(51) | 0.4(51) | 7.0 | 3.5(14) | 2700 | 1350 | 19.1 | 43.0 | 2.53(43) |
| r0e2 | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 3.5(14) | 5700 | 2850 | 19.1 | 31.7 | 3.75(43) |
| r0e4 | 0.17 | 9.86 | 1.23(52) | 0.4(51) | 7.0 | 3.5(14) | 10 000 | 5000 | 19.1 | 25.8 | 4.86(43) |
| r0e2 | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 3.5(14) | 5700 | 2850 | 19.1 | 31.7 | 3.75(43) |
| r0e2ba | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 1.0(14) | 5700 | 2850 | 234.4 | 48.9 | 1.61(43) |
| r0e2 | 0.13 | 9.69 | 4.12(51) | 0.4(51) | 7.0 | 3.5(14) | 5700 | 2850 | 19.1 | 31.7 | 3.75(43) |
| r0e2ea | 0.13 | 9.69 | 4.12(51) | 0.8(51) | 5.0 | 3.5(14) | 6800 | 3400 | 9.6 | 25.0 | 7.20(43) |
| r0e2eb | 0.13 | 9.69 | 4.12(51) | 1.2(51) | 4.1 | 3.5(14) | 8000 | 4000 | 6.4 | 21.6 | 1.03(44) |
| r0e2ec | 0.13 | 9.69 | 4.12(51) | 5.0(51) | 2.0 | 2.0(14) | 8000 | 4000 | 4.7 | 24.6 | 3.21(44) |
Notes. Numbers in parenthesis correspond to powers of ten. Each group of models (separated by a horizontal line) has a specific purpose. Models 5p11Bx2 and 5p11Bx2th address the influence of non-thermal processes. The reference magnetar model r0e2 is confronted to model r0e2n (no magnetar), to model r0e2s (narrow magnetar-power deposition profile), to models r0e1 and r0e4 (different explosion energies), to model r0e2ba (different magnetar field strength), and to models r0e2ea, r0e2eb, and r0e2ec (different magnetar spins). Also discussed is the influence of ejecta clumping for model r0e2 (Sect. 9).
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