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Table 4

Derived abundances for the stars in our sample.

HD HD HD
Species 74146 162586 162630 Sun

log(N/NT) [N/NT] σ (n) log(N/NT) [N/NT] σ (n) log(N/NT) [N/NT] σ (n) log(N/NT)Sun

He I –0.78 0.29 0.07 (9) –0.78 0.29 0.05 (8) –1.23 –0.16 0.08 (5) –1.07
C II –3.44 0.08 0.24 (5) –3.27 0.25 0.34 (5) –3.5 0.02 (2) –3.52
N II –3.69 0.43 (1) –4.12
O I –3.5 –0.29 0.01 (3) –3.21
Mg I –4.07 0.39 0.14 (4) –4.46
Mg II –4.87 –0.41 0.12 (4) –4.55 –0.09 0.06 (6) –4.36 0.1 0.06 (2) –4.46
Al I –5.56 0.01 (1) –5.57
Al II –6.2 –0.63 (1) –5.69 –0.12 (1) –5.26 0.31 (1) –5.57
Si II –4.92 –0.43 0.17 (6) –4.59 –0.09 0.05 (9) –4.42 0.07 0.08 (5) –4.49
S II –4.68 0.03 0.18 (10) –4.66 0.05 0.07 (7) –4.71
Ca II –6.45 –0.77 (1) –5.59 0.09 (1) –5.66 0.02 (1) –5.68
Sc II –9.02 –0.15 (1) –8.87
Ti II –6.84 0.18 0.21 (20) –6.98 0.04 0.18 (12) –7.02
Cr II –6.25 0.12 0.11 (16) –6.23 0.14 0.24 (8) –6.37
Fe I –4.41 0.13 0.12 (15) –4.44 0.1 0.14 (7) –4.54
Fe II –5.22 –0.68 0.22 (13) –4.57 –0.03 0.14 (60) –4.41 0.13 0.11 (16) –4.54
Ni II –5.79 0 0.15 (3) –5.41 0.38 0.29 (3) –5.79
Sr II –8.66 0.41 0.15 (2) –8.32 0.75 0.14 (2) –9.07

Notes. We use the same notation as in Table 3.

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