Table B.1.
Abundances pattern of selected elements in terms of [X/Fe].
| Mini/M⊙ | < log10(7Li)> | C | N | O | F | Ne | Na | Mg | Al | Si | P | S |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 3.0 | 2.50 | 4.30 | 4.97 | 2.55 | 4.30 | 3.50 | 3.29 | 3.22 | 2.40 | 1.36 | 1.69 | 4.0×10−2 |
| 3.0-dil | 1.47 | 3.27 | 3.93 | 1.52 | 3.27 | 2.46 | 2.26 | 2.18 | 1.38 | 0.48 | 0.73 | 3.8×10−3 |
| 4.0 | 1.43 | 3.55 | 5.03 | 2.31 | 3.34 | 3.22 | 3.19 | 3.00 | 2.48 | 1.22 | 1.72 | 4.2×10−2 |
| 4.0-dil | 0.65 | 2.68 | 4.16 | 1.44 | 2.47 | 2.34 | 2.31 | 2.13 | 1.62 | 0.49 | 0.89 | 5.9×10−3 |
| 5.0 | 0.89 | 3.44 | 4.98 | 2.29 | 2.90 | 2.94 | 2.92 | 2.93 | 2.57 | 1.13 | 1.71 | 5.7×10−2 |
| 5.0-dil | 0.33 | 2.66 | 4.20 | 1.53 | 2.13 | 2.17 | 2.15 | 2.16 | 1.81 | 0.49 | 0.98 | 1.0×10−2 |
| 6.0 | 0.29 | 3.37 | 4.63 | 2.03 | 2.34 | 2.37 | 2.37 | 2.62 | 2.33 | 0.94 | 1.60 | 4.2×10−2 |
| 6-0-dil | 0.08 | 2.67 | 3.93 | 1.35 | 1.65 | 1.68 | 1.68 | 1.92 | 1.64 | 0.41 | 0.94 | 8.8×10−3 |
| 7.0 | 0.12 | 2.79 | 4.14 | 1.50 | 1.80 | 1.46 | 1.23 | 1.60 | 1.52 | 0.58 | 0.51 | 6.9×10−3 |
| 7.0-dil | 0.03 | 2.15 | 3.50 | 0.90 | 1.18 | 0.86 | 0.67 | 0.99 | 0.92 | 0.21 | 0.18 | 1.6×10−3 |
| 7.5 | 1.67 | 2.74 | 4.16 | 1.63 | 1.47 | 1.34 | 0.95 | 1.52 | 1.34 | 0.40 | 0.53 | 4.2×10−3 |
| 7.5-dil | 1.08 | 2.13 | 3.54 | 1.04 | 0.89 | 0.78 | 0.46 | 0.94 | 0.78 | 0.13 | 0.19 | 1.0×10−3 |
Notes. Data are either given by the ejecta, or under the assumption that 1% of this matter was homogeneously diluted in the surface 0.2 M⊙ of an unevolved Z = 10−6 star. Lithium abundance is shown as < log10(7Li) > = Log10(N(Li)/N(H)) + 12. Stellar winds for these results are from Bloecker (1995), with parameter η = 0.02.
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