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Table 9.
Initial chemical abundances of our stellar evolutionary models.
| Element | Mass fraction | Reference |
|---|---|---|
| C | 20.82 × 10−5 | Kurt & Dufour (1998) |
| N | 3.28 × 10−5 | Kurt & Dufour (1998) |
| O | 113.07 × 10−5 | Kurt & Dufour (1998) |
| Mg | 9.32 × 10−5 | Trundle et al. (2007) |
| Hunter et al. (2007) | ||
| Si | 1.30 × 10−5 | Trundle et al. (2007) |
| Hunter et al. (2007) | ||
| Fe | 33.74 × 10−5 | Venn (1999) |
Notes. All elements that are not listed here correspond to the solar abundances from Asplund et al. (2005) scaled down by a factor of 1/5.
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