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Table 5
The abundances are measured with respect to H, and are tabulated with their associated uncertainties.
| Element | log (NX/NH) | Solar | # Lines |
|
|
|||
| He | < −2.20 | −1.07 | 2 |
| O | −3.77 ± 0.20 | −3.31 | 3 |
| Mg | −5.03 ± 0.15 | −4.40 | 1 |
| Si | −3.21 ± 0.30 | −4.49 | 5 |
| Ca | −6.19 ± 0.33 | −5.66 | 1 |
| Ti | −5.55 ± 0.50 | −7.05 | 7 |
| Cr | −3.86 ± 0.30 | −6.36 | 30 |
| Mn | −5.67 ± 0.20 | −6.57 | 2 |
| Fe | −3.10 ± 0.50 | −4.50 | 28 |
| Co | −4.51 ± 0.25 | −7.01 | 8 |
| Ni | −5.24 ± 0.20 | −5.78 | 1 |
| Sr | −7.78 ± 0.40 | −9.13 | 2 |
| La | −7.68 ± 0.16 | −10.9 | 2 |
| Ce | −6.86 ± 0.20 | −10.42 | 3 |
| Pr | −6.80 ± 0.25 | −11.28 | 4 |
| Nd | −6.54 ± 0.30 | −10.58 | 9 |
| Eu | −7.49 ± 0.20 | −11.48 | 3 |
Notes. For reference, the solar abundance ratio and the number of spectral lines modelled are also shown.
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