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Table C.1
Stellar abundances of Fe, Sr, Y, Zr, Pd, Ag, Ba, and Eu for dwarfs.
| Star | [Fe/H] | [Sr/Fe] | [Y/Fe] | [Zr/Fe] | [Pd/Fe] | [Ag/Fe] | [Ba/Fe] | [Eu/Fe] |
|
|
||||||||
| BD+09 2190 | –2.60 | – | −0.28 ± 0.17 | −0.02 ± 0.14 | 0.72 ± 0.27 | – | – | – |
| BD-13 3442 | –2.56 | 0.21 ± 0.14 | −0.02 ± 0.13 | 0.44 ± 0.18 | – | – | – | – |
| CD-30 18140 | –1.92 | 0.15 ± 0.11 | 0.1 ± 0.12 | 0.47 ± 0.14 | – | – | −0.10 ± 0.25 | – |
| CD-33 3337 | –1.55 | 0.22 ± 0.11 | 0.01 ± 0.13 | 0.27 ± 0.17 | 0.19 ± 0.27 | 0.27 ± 0.25 | 0.18 ± 0.14 | – |
| CD-45 3283 | –0.99 | −0.15 ± 0.30 | 0.03 ± 0.15 | 0.14 ± 0.17 | 0.52 ± 0.19 | 0.38 ± 0.25 | 0.32 ± 0.15 | 0.78 ± 0.17 |
| CD-57 1633 | –1.01 | 0.00 ± 0.10 | −0.23 ± 0.12 | – | 0.17 ± 0.23 | 0.20 ± 0.26 | 0.13 ± 0.14 | 0.55 ± 0.22 |
| HD 3567 | –1.33 | −0.1 ± 0.20 | −0.18 ± 0.19 | 0.27 ± 0.17 | 0.29 ± 0.20 | 0.53 ± 0.25 | 0.26 ± 0.17 | 0.70 ± 0.18 |
| HD 19445 | –2.13 | 0.13 ± 0.11 | −0.1 ± 0.12 | 0.29 ± 0.15 | 0.00 ± 0.27 | – | −0.02 ± 0.14 | 0.37 ± 0.23 |
| HD 22879 | –0.95 | 0.33 ± 0.14 | −0.06 ± 0.12 | 0.19 ± 0.17 | 0.17 ± 0.21 | 0.00 ± 0.26 | −0.18 ± 0.18 | 0.45 ± 0.2 |
| HD 25704 | –1.12 | 0.30 ± 0.11 | −0.05 ± 0.12 | −0.02 ± 0.17 | 0.07 ± 0.21 | 0.09 ± 0.26 | 0.21 ± 0.15 | 0.48 ± 0.17 |
| HD 63077 | –1.05 | 0.36 ± 0.25 | 0.06 ± 0.13 | 0.06 ± 0.17 | 0.00 ± 0.22 | 0.07 ± 0.26 | 0.22 ± 0.15 | 0.43 ± 0.17 |
| HD 63598 | –0.990 | 0.41 ± 0.14 | 0.09 ± 0.12 | 0.20 ± 0.22 | 0.09 ± 0.19 | −0.07 ± 0.26 | 0.19 ± 0.15 | 0.65 ± 0.27 |
| HD 76932 | –0.97 | < 0.27 | −0.07 ± 0.13 | 0.19 ± 0.17 | 0.20 ± 0.20 | 0.25 ± 0.25 | 0.30 ± 0.15 | 0.41 ± 0.16 |
| HD 103723 | –0.85 | 0.04 ± 0.13 | −0.27 ± 0.15 | 0.05 ± 0.17 | 0.29 ± 0.19 | 0.21 ± 0.25 | 0.17 ± 0.15 | 0.43 ± 0.16 |
| HD 105004 | –0.84 | 0.10 ± 0.10 | −0.19 ± 0.12 | 0.02 ± 0.17 | 0.12 ± 0.19 | 0.01 ± 0.27 | 0.17 ± 0.18 | 0.26 ± 0.20 |
| HD 106038 | –1.48 | 0.56 ± 0.17 | 0.54 ± 0.14 | 0.68 ± 0.17 | 0.32 ± 0.21 | 0.14 ± 0.25 | 0.76 ± 0.17 | 0.45 ± 0.16 |
| HD 113679 | –0.63 | < 0.44 | 0.08 ± 0.12 | 0.22 ± 0.17 | 0.14 ± 0.19 | 0.08 ± 0.25 | 0.25 ± 0.15 | 0.08 ± 0.21 |
| HD 111980 | –1.32 | 0.45 ± 0.22 | 0.23 ± 0.13 | 0.44 ± 0.17 | 0.17 ± 0.21 | 0.10 ± 0.25 | 0.48 ± 0.15 | < 0.5 |
| HD 116064 | –2.17 | – | 0.00 ± 0.13 | 0.33 ± 0.14 | 0.37 ± 0.21 | – | −0.36 ± 0.17 | – |
| HD 120559 | –1.31 | 0.22 ± 0.12 | 0.25 ± 0.15 | 0.34 ± 0.17 | 0.44 ± 0.21 | 0.48 ± 0.25 | 0.22 ± 0.17 | 0.71 ± 0.17 |
| HD 121004 | –0.73 | 0.40 ± 0.12 | 0.16 ± 0.12 | 0.51 ± 0.17 | 0.32 ± 0.19 | 0.16 ± 0.25 | 0.36 ± 0.18 | 0.50 ± 0.19 |
| HD 122196 | –1.81 | 0.03 ± 0.14 | −0.15 ± 0.12 | 0.20 ± 0.16 | 0.02 ± 0.27 | < 0.22 | 0.02 ± 0.16 | 0.22 ± 0.18 |
| HD 126681 | –1.28 | 0.20 ± 0.19 | 0.34 ± 0.12 | 0.56 ± 0.17 | 0.51 ± 0.21 | 0.28 ± 0.25 | 0.55 ± 0.15 | 0.47 ± 0.17 |
| HD 132475 | –1.52 | 0.34 ± 0.11 | 0.17 ± 0.15 | 0.46 ± 0.17 | 0.34 ± 0.19 | 0.20 ± 0.26 | 0.40 ± 0.15 | 0.43 ± 0.16 |
| HD 140283 | –2.58 | −0.27 ± 0.10 | −0.48 ± 0.12 | −0.20 ± 0.14 | – | – | < − 0.62 | – |
| HD 160617 | –1.83 | 0.04 ± 0.14 | −0.03 ± 0.12 | 0.19 ± 0.21 | 0.42 ± 0.21 | < 0.35 | 0.41 ± 0.16 | – |
| HD 166913 | –1.93 | 0.47 ± 0.15 | 0.39 ± 0.14 | 0.65 ± 0.18 | 0.42 ± 0.23 | < 0.63 | 0.62 ± 0.14 | 0.61 ± 0.16 |
| HD 175179 | –0.72 | < 1.28 | < 0.95 | 0.17 ± 0.17 | 0.12 ± 0.20 | 0.09 ± 0.26 | 0.45 ± 0.14 | 0.20 ± 0.16 |
| HD 188510 | –1.58 | −0.04 ± 0.14 | −0.16 ± 0.13 | 0.18 ± 0.17 | 0.32 ± 0.19 | 0.19 ± 0.26 | 0.13 ± 0.14 | 0.40 ± 0.18 |
| HD 189558 | –1.18 | −0.70 ± 0.14 | 0.15 ± 0.13 | 0.44 ± 0.17 | 0.30 ± 0.21 | 0.16 ± 0.25 | 0.32 ± 0.17 | 0.39 ± 0.16 |
| HD 195633 | –0.71 | < 1.11 | < 0.66 | −0.14 ± 0.17 | −0.13 ± 0.20 | −0.03 ± 0.28 | 0.10 ± 0.16 | < 0.1 |
| HD 205650 | –1.19 | −0.02 ± 0.25 | 0.05 ± 0.13 | 0.19 ± 0.17 | 0.22 ± 0.21 | 0.14 ± 0.25 | 0.20 ± 0.14 | 0.45 ± 0.16 |
| HD 213657 | –2.01 | 0.04 ± 0.11 | −0.05 ± 0.12 | 0.37 ± 0.15 | 0.22 ± 0.27 | < 0.53 | −0.03 ± 0.15 | – |
| HD 298986 | –1.48 | −0.03 ± 0.17 | −0.09 ± 0.14 | 0.23 ± 0.17 | 0.32 ± 0.19 | 0.43 ± 0.28 | 0.14 ± 0.16 | 0.54 ± 0.16 |
| G 01-039 | –2.27 | 0.16 ± 0.10 | −0.07 ± 0.12 | 0.29 ± 0.14 | – | – | – | – |
| G 05-040 | –0.93 | < 1.29 | < 1.09 | 0.37 ± 0.17 | 0.16 ± 0.21 | 0.17 ± 0.26 | 0.35 ± 0.14 | < 0.5 |
| G 20-024 | –1.90 | 0.22 ± 0.11 | 0.17 ± 0.12 | 0.56 ± 0.15 | 0.77 ± 0.27 | – | 0.32 ± 0.14 | – |
| G 64-012 | –3.10 | −0.05 ± 0.10 | 0.02 ± 0.13 | – | – | – | −0.35 ± 0.16 | – |
| G 64-037 | –3.16 | −0.06 ± 0.10 | 0.03 ± 0.13 | 0.52 ± 0.14 | – | – | – | – |
| G 88-032 | –2.53 | – | −0.14 ± 0.13 | 0.25 ± 0.14 | – | – | – | – |
| G 88-040 | –0.89 | 0.04 ± 0.10 | −0.27 ± 0.15 | 0.02 ± 0.17 | 0.12 ± 0.19 | 0.03 ± 0.26 | 0.05 ± 0.14 | 0.32 ± 0.16 |
| G183-011 | –2.12 | – | −0.24 ± 0.12 | 0.18 ± 0.17 | – | – | – | – |
Notes. The “ < ” indicates that the abundance is an upper limit.
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