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Table 3
Abundance estimates from the mean low-〈B〉 HARPS spectrum of HD 57372.
| Atom/Ion | Z | [X/H] (dex) | N |
|---|---|---|---|
| He I | 2.00 | −0.05 ± 0.02 | 1 |
| C II | 6.01 | 0.81 ± 0.05 | 3 |
| N II | 7.01 | 1.41 ± 0.38 | 6 |
| O I | 8.00 | 1.00 ± 0.14 | 3 |
| O II | 8.01 | 1.73 ± 0.11 | 5 |
| Ne I | 10.00 | 0.35 ± 0.19 | 4 |
| Mg II | 12.01 | 0.96 ± 0.20 | 10 |
| Al II | 13.01 | 0.73 ± 0.16 | 5 |
| Al III | 13.02 | 1.52 ± 0.16 | 5 |
| Si II | 14.01 | 1.83 ± 0.28 | 36 |
| Si III | 14.02 | 2.63 ± 0.05 | 4 |
| P II | 15.01 | 0.80 ± 0.04 | 2 |
| S II | 16.01 | 1.42 ± 0.24 | 33 |
| Cl II | 17.01 | 3.14 ± 0.35 | 27 |
| Ca II | 20.01 | 1.92 ± 0.25 | 9 |
| Sc II | 21.01 | 2.13 ± 0.12 | 5 |
| Ti II | 22.01 | 2.16 ± 0.29 | 38 |
| V II | 23.01 | 0.86 ± 0.06 | 2 |
| Cr II | 24.01 | 1.71 ± 0.24 | 34 |
| Mn II | 25.01 | 0.76 ± 0.00 | 2 |
| Fe II | 26.01 | 1.61 ± 0.18 | 64 |
| Fe III | 26.02 | 2.09 ± 0.22 | 9 |
| Co II | 27.01 | 1.92 ± 0.06 | 2 |
| Ni II | 28.01 | 0.47 ± 0.34 | 2 |
| Sr II | 38.01 | 2.94 ± 0.04 | 2 |
| Ce III | 58.02 | 3.84 ± 0.08 | 2 |
| Pr III | 59.02 | 3.87 ± 0.14 | 3 |
| Nd III | 60.02 | 4.09 ± 0.20 | 28 |
| Tb III | 65.02 | 3.94 ± 0.36 | 7 |
| Dy III | 66.02 | 3.96 ± 0.35 | 19 |
| Ho III | 67.02 | 3.59 ± 0.05 | 3 |
| Er III | 68.02 | 4.13 ± 0.20 | 8 |
Notes. The abundances are given relative to the solar abundances presented by Asplund et al. (2021). The number of spectral lines used for the abundance determination is presented in the last column.
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