Table A.24.
Summary of important fractional powers that characterize our He-star explosion models computed with CMFGEN.
| Model | f(He-sh) | f(O-sh) | f(Si-sh) | f(Fe-sh) | fpositron | fabs |
|---|---|---|---|---|---|---|
| he2p6 | 0.71 | 0.12 | 0.14 | 0.03 | 0.17 | 0.19 |
| he2p9 | 0.52 | 0.15 | 0.28 | 0.06 | 0.28 | 0.11 |
| he3p3 | 0.30 | 0.32 | 0.20 | 0.19 | 0.21 | 0.15 |
| he3p5 | 0.33 | 0.38 | 0.23 | 0.06 | 0.16 | 0.20 |
| he4p0 | 0.25 | 0.47 | 0.20 | 0.08 | 0.16 | 0.19 |
| he4p5 | 0.22 | 0.41 | 0.12 | 0.26 | 0.21 | 0.15 |
| he5p0 | 0.16 | 0.47 | 0.08 | 0.29 | 0.21 | 0.15 |
| he6p0 | 0.16 | 0.58 | 0.09 | 0.17 | 0.12 | 0.26 |
| he7p0 | 0.03 | 0.70 | 0.08 | 0.20 | 0.11 | 0.27 |
| he8p0 | 0.02 | 0.80 | 0.06 | 0.12 | 0.06 | 0.55 |
| he12p0 | 0.00 | 0.81 | 0.09 | 0.10 | 0.04 | 0.76 |
| he5p0x1p5 | 0.09 | 0.44 | 0.11 | 0.36 | 0.28 | 0.11 |
| he6p0x1p5 | 0.06 | 0.57 | 0.07 | 0.30 | 0.20 | 0.16 |
| he8p0x1p5 | 0.03 | 0.71 | 0.08 | 0.19 | 0.12 | 0.26 |
| he9p0x1p5 | 0.00 | 0.73 | 0.08 | 0.19 | 0.09 | 0.34 |
| he10p0x1p5 | 0.00 | 0.74 | 0.08 | 0.18 | 0.10 | 0.31 |
| he11p0x1p5 | 0.00 | 0.85 | 0.11 | 0.03 | 0.09 | 0.34 |
| he12p0x1p5 | 0.00 | 0.78 | 0.09 | 0.14 | 0.07 | 0.46 |
| he13p0x1p5 | 0.00 | 0.73 | 0.08 | 0.18 | 0.08 | 0.40 |
| he10p0x2p0 | 0.00 | 0.64 | 0.11 | 0.25 | 0.17 | 0.18 |
Notes: Fractional decay powers absorbed in the He-rich shell, the O-rich shell, the Si-rich shell, the Fe-rich shell, and then the fractional decay power absorbed that arises from positrons, and finally the fraction of the total decay power emitted that is absorbed in the ejecta. The SN age is 200 d. The models are he2p6 to he12p0 (nominal mass loss rate; x1p0 series), he5p0x1p5 to he13p0x1p5 (50% enhancement in mass loss rate; x1p5 series), and model he10p0x2p0 (100% enhancement in mass loss rate; x2p0 series).
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