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Table 2.
Mean abundance as derived from BACCHUS for elements which have more than one line.
| APOGEE ID | 2M18032356− | 2M18033819− | 2M18033965- | 2M18034052− | 2M18033660− |
|---|---|---|---|---|---|
| 3001588 | 3000515 | 3000521 | 3003281 | 3002164 | |
| Teff (K) | 3977.2 | 4378.1 | 4555.8 | 4492.3 | 5021.1 |
| log g (dex) | 0.50 | 1.09 | 1.35 | 1.26 | 1.99 |
| ξt (km s−1) | 2.46 | 2.67 | 2.43 | 1.92 | 1.37 |
| [Fe/H] | −1.20 | −0.97 | −0.99 | −0.97 | −1.08 |
| [C/Fe] | −0.48 | −0.33 | −0.29 | −0.24 | ... |
| [N/Fe] | 1.29 | 1.30 | 1.03 | 1.20 | 1.13 |
| [O/Fe] | 0.39 | 0.30 | 0.29 | 0.35 | ... |
| [Al/Fe] | 0.38 | 0.77 | 0.39 | 0.93 | 0.39 |
| [Mg/Fe] | 0.16 | 0.04 | 0.05 | 0.05 | 0.33 |
| [Si/Fe] | 0.28 | 0.17 | 0.18 | 0.37 | 0.51 |
| [Ce/Fe] | 0.09 | 0.23 | ... | ... | ... |
Notes. The Solar reference abundances are from Asplund et al. (2005), except for Ce, which is taken from Grevesse et al. (2015).
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