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Table 4
Results of various SN fits to the proto-solar abundance ratios adapted from Lodders et al. (2009).
| SNcc | SNIa |
|
χ2/ d.o.f. |
|
|
|||
| Nomoto | Classical | ||
|
|
|||
| Z0.02 | WDD2 | 0.20 | 61.0/16 |
| Z0.02 | CDD2 | 0.19 | 61.8/16 |
| Z0.02 | WDD3 | 0.18 | 62.7/16 |
| Z0.02 | W70 | 0.19 | 72.3/16 |
| Z0.008 | WDD3 | 0.18 | 75.6/16 |
|
|
|||
| Nomoto | Bravo | ||
|
|
|||
| Z0.02 | DDTc | 0.20 | 64.5/16 |
| Z0.02 | DDTa | 0.15 | 66.2/16 |
| Z0.008 | DDTa | 0.15 | 77.6/16 |
| Z0.008 | DDTc | 0.21 | 80.0/16 |
| Z0.004 | DDTa | 0.16 | 94.2/16 |
|
|
|||
| Nomoto | 2D | ||
|
|
|||
| Z0.02 | O-DDT | 0.24 | 67.8/16 |
| Z0.008 | O-DDT | 0.25 | 81.4/16 |
| Z0.004 | O-DDT | 0.27 | 97.1/16 |
| Z0.001 | O-DDT | 0.30 | 99.5/16 |
| Z0_cut | O-DDT | 0.28 | 111.5/16 |
|
|
|||
| Nomoto | 3D | ||
|
|
|||
| Z0.02 | N100H | 0.18 | 62.0/16 |
| Z0.02 | N40 | 0.20 | 63.9/16 |
| Z0.02 | N100 | 0.21 | 64.1/16 |
| Z0.02 | N20 | 0.17 | 64.4/16 |
| Z0.02 | N150 | 0.22 | 64.6/16 |
Notes. Only one SNIa and one SNcc model have been fitted, and for each case we only show the five best fits (sorted by increasing χ2/ d.o.f.).
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