Table 2
Determined absolute abundances A(X) and solar- and metallicity-normalised abundances [X/Fe] of the Z06-star.
| Species | [X/Fe] | Reference | |
|---|---|---|---|
| C | 7.63 | −0.10 | Ryde et al. (2010) |
| N | 7.34 | 0.21 | Ryde et al. (2010) |
| O I | 8.47 | 0.48 | Jönsson et al. (2017b) |
| Na I | 5.67 | −0.08 | Johnson et al. (2014) |
| Mg I | 7.27 | 0.47 | Jönsson et al. (2017b) |
| AI I | 6.16 | 0.27 | Johnson et al. (2014) |
| Si I | 7.21 | 0.24 | Johnson et al. (2014) |
| Ca I | 5.88 | 0.25 | Jönsson et al. (2017b) |
| Sc II | 2.57 | 0.08 | Lomaeva et al. (2019) |
| Ti I | 4.43 | 0.19 | Jönsson et al. (2017b) |
| V I | 3.34 | 0.12 | Lomaeva et al. (2019) |
| Cr I | 4.48 | -0.11 | Lomaeva et al. (2019) |
| Co I | 4.40 | 0.14 | Lomaeva et al. (2019) |
| Ni I | 5.57 | 0.04 | Lomaeva et al. (2019) |
| Zr I | 2.35 | 0.43 | Forsberg et al. (2019) |
| Mo I | 1.87 | 0.62 | Forsberg et al. (2022) |
| Ba II | 2.33 | 0.78 | Van der Swaelmen et al. (2016) |
| La II | 0.93 | 0.42* | Forsberg et al. (2019) |
| Ce II | 1.11 | 0.22* | Forsberg et al. (2019) |
| Nd II | 1.15 | 0.32 | Van der Swaelmen et al. (2016) |
| Eu II | 0.73 | 0.78* | Forsberg et al. (2019) |
Notes. The Jönsson series, Jönsson et al. (2017b); Lomaeva et al. (2019); Forsberg et al. (2019, 2022) uses the solar values in the series of Scott et al. (2015a,b); Grevesse et al. (2015). For elements not determined in that series, we complement with values from Ryde et al. (2010); Johnson et al. (2014); Van der Swaelmen et al. (2016). The C and N abundances are from molecular CO and CN (Ryde et al. 2010). La, Ce, and Eu have been decreased by 0.05, 0.01, and 0.10 dex, as described in Sect. 3.1.
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