Table E.1.
[V/Fe] abundance ratios determined in the sample of three RGB stars from our target sample with the highest [Na/Fe] abundance ratios (columns 2, 4, and 6). The star IDs are given in the first row of the table. The first column shows the central wavelengths of the V I spectral lines. Columns 3, 5, and 7 (marked with an asterisk) show the [V/Fe] abundance ratios that were recalculated with log gf values, Fe and V solar abundances, and the Fe abundances of individual target stars taken from Ernandes et al. (2018).
| 00241344-7211263 | s17657 | s5270 | ||||
|---|---|---|---|---|---|---|
| λ, nm | [V/Fe] | [V/Fe]* | [V/Fe] | [V/Fe]* | [V/Fe] | [V/Fe]* |
| 570.3560 | 0.21 | −0.06 | 0.28 | 0.13 | 0.27 | 0.01 |
| 608.1440 | 0.32 | 0.08 | 0.32 | 0.20 | 0.34 | 0.11 |
| 609.0220 | 0.22 | −0.15 | 0.31 | 0.06 | 0.28 | −0.08 |
| 611.9520 | 0.23 | −0.16 | 0.29 | 0.02 | 0.28 | −0.10 |
| 619.9190 | 0.33 | 0.04 | 0.29 | 0.12 | 0.35 | 0.07 |
| 624.3100 | 0.27 | 0.06 | – | – | 0.30 | 0.10 |
| 625.1820 | 0.28 | −0.06 | 0.31 | 0.09 | 0.30 | −0.03 |
| 627.4650 | 0.29 | 0.00 | 0.30 | 0.13 | 0.28 | 0.00 |
| 650.4165 | 0.39 | – | 0.34 | – | 0.40 | – |
| Average | 0.27 ± 0.04 | −0.03 ± 0.09 | 0.30 ± 0.01 | 0.11 ± 0.05 | 0.30 ± 0.03 | 0.01 ± 0.07 |
Note: The average values in the last row do not include the 650.4165 nm line because it was not used by Ernandes et al. (2018). The errors denote the standard deviation due to the star-to-star abundance variation.
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