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Table 1
Parameters of the model shown in Fig. 2, with respect to the solar abundances from Asplund et al. (2009) provided for comparison.
| Parameter | Value | + 1σ | −1σ | Unit | × Solar |
|
|
|||||
| T eff | 27 450 | 200 | 200 | K | |
| log g | 5.438 | 0.028 | 0.033 | dex | |
| log n(He) /n(H) | –2.56 | 0.03 | 0.07 | dex | 0.032 |
| log n(C) /n(H) | –5.04 | 0.26 | 0.55 | dex | 0.034 |
| log n(N) /n(H) | –4.65 | 0.11 | 0.34 | dex | 0.331 |
| log n(O) /n(H) | –4.07 | 0.10 | 0.16 | dex | 0.172 |
| log n(Si) /n(H) | –5.25 | 0.20 | 0.21 | dex | 0.175 |
| log n(S) /n(H) | –5.36> | dex | 0.33> | ||
| log n(Fe) /n(H) | –4.22 | 0.18 | 0.25 | dex | 1.920 |
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