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Table 5.
Abundances of standard stars.
| G 112-43 |
|||||
|---|---|---|---|---|---|
| N | [X/H] | σ | [X/Fe] | σ | |
| Fe I | 100 | −1.254 | 0.022 | … | … |
| Fe II | 10 | −1.256 | 0.019 | … | … |
| Na I | 3 | −1.423 | 0.076 | −0.169 | 0.074 |
| Mg I | 5 | −1.075 | 0.038 | 0.179 | 0.036 |
| Si I | 5 | −1.035 | 0.025 | 0.219 | 0.027 |
| Ca I | 16 | −0.977 | 0.028 | 0.278 | 0.025 |
| Ti I | 11 | −0.951 | 0.044 | 0.303 | 0.037 |
| Ti II | 7 | −0.914 | 0.035 | 0.343 | 0.033 |
| Cr I | 6 | −1.200 | 0.058 | 0.055 | 0.052 |
| Mn I | 4 | −1.527 | 0.071 | −0.273 | 0.069 |
| Ni I | 20 | −1.185 | 0.029 | 0.069 | 0.025 |
| Zn I | 2 | −0.940 | 0.036 | 0.315 | 0.035 |
| Y II | 2 | −1.390 | 0.037 | −0.134 | 0.035 |
| Ba II | 3 | −1.584 | 0.044 | −0.328 | 0.041 |
| CD−48°02445 |
|||||
| N | [X/H] | σ | [X/Fe] | σ | |
| Fe I | 111 | −1.814 | 0.025 | … | … |
| Fe II | 11 | −1.829 | 0.021 | … | … |
| Na I | 2 | −2.091 | 0.082 | −0.276 | 0.079 |
| Mg I | 6 | −1.563 | 0.035 | 0.251 | 0.033 |
| Si I | 2 | −1.414 | 0.111 | 0.400 | 0.112 |
| Ca I | 23 | −1.461 | 0.026 | 0.353 | 0.025 |
| Ti I | 10 | −1.372 | 0.051 | 0.442 | 0.043 |
| Ti II | 14 | −1.540 | 0.032 | 0.289 | 0.031 |
| Cr I | 5 | −1.786 | 0.049 | 0.028 | 0.041 |
| Mn I | 7 | −2.161 | 0.048 | −0.346 | 0.042 |
| Ni I | 13 | −1.844 | 0.044 | −0.029 | 0.040 |
| Zn I | 1 | −1.657 | 0.045 | 0.158 | 0.043 |
| Y II | 2 | −1.749 | 0.043 | 0.080 | 0.040 |
| Ba II | 4 | −1.985 | 0.044 | −0.156 | 0.041 |
| HD 59392 |
|||||
| N | [X/H] | σ | [X/Fe] | σ | |
| Fe I | 134 | (−1.600) | … | (…) | … |
| Fe II | 20 | (−1.600) | … | (…) | … |
| Na I | 4 | (−1.750) | … | (−0.150) | … |
| Mg I | 7 | (−1.320) | … | (0.280) | … |
| Si I | 8 | (−1.330) | … | (0.270) | … |
| Ca I | 23 | (−1.220) | … | (0.380) | … |
| Ti I | 16 | (−1.270) | … | (0.330) | … |
| Ti II | 14 | (−1.270) | … | (0.330) | … |
| Cr I | 6 | (−1.600) | … | (0.000) | … |
| Mn I | 8 | (−1.960) | … | (−0.360) | … |
| Ni I | 26 | (−1.610) | … | (−0.010) | … |
| Zn I | 2 | (−1.460) | … | (0.140) | … |
| Y II | 2 | (−1.470) | … | (0.130) | … |
| Ba II | 4 | (−1.670) | … | (−0.070) | … |
Notes. The abundance of HD 59392 is identical to NS 10 since this is the reference star in our analysis.
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