Free Access

Table A.2

LTE and non-LTE copper abundance ratios [Cu/Fe] for stars with NOT/FIES spectra.

Star Teff (K) log g [Fe/H] ξ [α/Fe] 5105 Å 5218 Å 5782 Å [Cu/Fe] Class LFS

G13-38 5263 4.54 −0.88 0.90 0.32 −0.04 −0.11 −0.11 −0.09 ± 0.04 high-α L
0.00 −0.11 −0.08 −0.06 ± 0.06 N
G15-23 5297 4.57 −1.10 1.00 0.34 −0.16 −0.17 −0.19 −0.17 ± 0.02 high-α L
−0.11 −0.17 −0.15 −0.14 ± 0.03 N
G24-13 5673 4.31 −0.72 1.00 0.29 −0.16 −0.20 −0.14 −0.17 ± 0.03 high-α L
−0.11 −0.18 −0.09 −0.13 ± 0.05 N
G31-55 5638 4.30 −1.10 1.40 0.29 −0.25 ... −0.23 −0.24 ± 0.01 high-α L
−0.16 ... −0.15 −0.16 ± 0.01 N
G49-19 5772 4.25 −0.55 1.20 0.27 −0.07 −0.07 −0.06 −0.07 ± 0.01 high-α L
−0.01 −0.04 −0.01 −0.02 ± 0.02 N
G56-30 5830 4.26 −0.89 1.30 0.11 −0.50 −0.47 −0.49 −0.49 ± 0.02 low-α L
−0.42 −0.43 −0.39 −0.41 ± 0.02 N
G56-36 5933 4.28 −0.94 1.40 0.20 −0.37 −0.41 −0.35 −0.38 ± 0.03 low-α L
−0.27 −0.36 −0.26 −0.30 ± 0.06 N
G57-07 5676 4.25 −0.47 1.10 0.31 −0.05 −0.07 −0.03 −0.05 ± 0.02 high-α L
−0.01 −0.05 0.01 −0.02 ± 0.03 N
G74-32 5772 4.36 −0.72 1.10 0.30 −0.14 −0.10 −0.13 −0.12 ± 0.02 high-α L
−0.08 −0.07 −0.07 −0.07 ± 0.01 N
G75-31 6010 4.02 −1.03 1.40 0.20 −0.70 ... ... −0.70 ± 0.00 low-α L
−0.56 ... ... −0.56 ± 0.00 N
G81-02 5859 4.19 −0.69 1.30 0.19 −0.20 −0.13 −0.26 −0.20 ± 0.07 high-α L
−0.13 −0.09 −0.19 −0.14 ± 0.05 N
G85-13 5628 4.38 −0.59 1.00 0.28 −0.02 −0.05 −0.04 −0.04 ± 0.02 high-α L
0.03 −0.03 0.00 0.00 ± 0.03 N
G87-13 6085 4.13 −1.09 1.50 0.20 −0.56 ... ... −0.56 ± 0.00 low-α L
−0.41 ... ... −0.41 ± 0.00 N
G94-49 5373 4.50 −0.80 1.10 0.31 −0.01 −0.09 −0.09 −0.06 ± 0.05 high-α L
0.02 −0.08 −0.06 −0.04 ± 0.05 N
G96-20 6293 4.41 −0.89 1.50 0.28 −0.09 −0.10 ... −0.09 ± 0.01 high-α L
0.03 −0.01 ... 0.01 ± 0.03 N
G98-53 5848 4.23 −0.87 1.30 0.19 −0.34 −0.26 −0.27 −0.29 ± 0.04 low-α L
−0.25 −0.22 −0.19 −0.22 ± 0.03 N
G99-21 5487 4.39 −0.67 0.90 0.29 −0.08 −0.09 −0.10 −0.09 ± 0.01 high-α L
−0.04 −0.08 −0.06 −0.06 ± 0.02 N
G127-26 5791 4.14 −0.53 1.20 0.24 −0.08 −0.09 −0.12 −0.10 ± 0.02 high-α L
−0.02 −0.07 −0.07 −0.05 ± 0.03 N
G150-40 5968 4.09 −0.81 1.40 0.16 −0.34 ... ... −0.34 ± 0.00 low-α L
−0.24 ... ... −0.24 ± 0.00 N
G170-56 5994 4.12 −0.92 1.50 0.17 −0.44 −0.45 −0.37 −0.42 ± 0.04 low-α L
−0.33 −0.38 −0.26 −0.32 ± 0.06 N
G172-61 5225 4.47 −1.00 0.90 0.19 −0.32 −0.37 −0.33 −0.34 ± 0.03 low-α L
−0.28 −0.37 −0.30 −0.32 ± 0.05 N
G176-53 5523 4.48 −1.34 1.00 0.18 −0.66 ... ... −0.66 ± 0.00 low-α L
−0.59 ... ... −0.59 ± 0.00 N
G180-24 6004 4.21 −1.39 1.50 0.33 −0.46 ... ... −0.46 ± 0.00 high-α L
−0.27 ... ... −0.27 ± 0.00 N
G187-18 5607 4.39 −0.67 1.10 0.26 −0.08 −0.08 −0.11 −0.09 ± 0.02 high-α L
−0.03 −0.06 −0.07 −0.05 ± 0.02 N
G232-18 5559 4.48 −0.93 1.30 0.32 −0.25 −0.27 −0.21 −0.24 ± 0.03 high-α L
−0.19 −0.25 −0.15 −0.20 ± 0.05 N
HD 148816a 5840 4.14 −0.70 1.40 0.26 −0.11 −0.16 −0.12 −0.13 ± 0.03 high-α L
−0.03 −0.12 −0.05 −0.07 ± 0.05 N
HD 159482 5737 4.31 −0.73 1.30 0.30 −0.10 −0.11 −0.10 −0.10 ± 0.01 high-α L
−0.03 −0.08 −0.04 −0.05 ± 0.03 N
HD 160693 5714 4.27 −0.49 1.10 0.19 −0.09 −0.06 −0.14 −0.10 ± 0.04 high-α L
−0.04 −0.04 −0.10 −0.06 ± 0.03 N
HD 177095 5349 4.39 −0.74 0.90 0.31 −0.09 −0.10 −0.16 −0.12 ± 0.04 high-α L
−0.05 −0.09 −0.13 −0.09 ± 0.04 N
HD 179626a 5855 4.19 −1.00 1.40 0.32 −0.33 −0.27 −0.22 −0.27 ± 0.06 high-α L
−0.22 −0.21 −0.12 −0.18 ± 0.06 N
HD 189558a 5623 3.81 −1.12 1.40 0.35 −0.44 −0.40 −0.37 −0.40 ± 0.04 TD L
−0.32 −0.34 −0.25 −0.30 ± 0.05 N
HD 193901a 5676 4.41 −1.07 1.40 0.17 −0.65 −0.60 −0.54 −0.60 ± 0.06 low-α L
−0.57 −0.57 −0.47 −0.54 ± 0.06 N
HD 194598a 5926 4.32 −1.08 1.40 0.20 −0.43 −0.44 ... −0.44 ± 0.01 low-α L
−0.32 −0.38 ... −0.35 ± 0.04 N
HD 230409 5318 4.54 −0.85 1.10 0.27 0.00 −0.02 −0.07 −0.03 ± 0.04 high-α L
0.04 −0.01 −0.04 −0.00 ± 0.04 N
HD 237822 5603 4.33 −0.45 1.10 0.29 0.02 0.02 −0.02 0.01 ± 0.02 high-α L
0.06 0.03 0.02 0.04 ± 0.02 N
HD 250792A 5489 4.47 −1.01 1.10 0.24 −0.54 −0.48 −0.51 −0.51 ± 0.03 low-α L
−0.49 −0.47 −0.46 −0.47 ± 0.02 N

Notes. Table A.2 is in the same format as Table A.1. The stars without available copper abundance are not listed in the table.

(a)

The stars that also have VLT/UVES spectra.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.