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Table 3
Average elemental abudances measured for both Pal1-I and the Sun.
Element | Ion | ϵ | [X/Fe I] | σ | Lines | ϵ | σ | Lines | ϵ(Sun) | [X/H]Sun |
Pal1-I | Sun | GS98 | t.w.-GS98 | |||||||
|
||||||||||
Al | I | 5.98 | +0.25 | 0.02 | 2 | 6.22 | 0.04 | 2 | 6.47 | −0.25 |
Ba | II | 2.00 | +0.24 | 0.02 | 2 | 2.25 | 0.07 | 2 | 2.13 | +0.12 |
Ca | I | 5.93 | +0.04 | 0.14 | 8 | 6.38 | 0.13 | 6 | 6.36 | +0.02 |
Co | I | 4.42 | −0.06 | – | 1 | 4.97 | – | 1 | 4.92 | +0.05 |
Cr | I | 4.93 | −0.23 | 0.20 | 5 | 5.65 | 0.07 | 4 | 5.67 | −0.02 |
Fe | I | 7.09 | [FeI/H] = −0.49 | 0.18 | 108 | 7.58 | 0.12 | 95 | 7.50 | +0.08 |
Fe | II | 7.08 | [FeII/H] = −0.53 | 0.17 | 7 | 7.61 | 0.06 | 7 | 7.50 | +0.11 |
La | II | 0.93 | +0.29 | 0.05 | 2 | 1.13 | – | 0 | 1.13 | – |
Mg | I | 7.11 | +0.11 | 0.08 | 3 | 7.49 | 0.17 | 3 | 7.58 | −0.09 |
Mn | I | 4.63 | −0.22 | – | 1 | 5.34 | – | 1 | 5.39 | −0.05 |
Na | I | 6.07 | +0.38 | 0.12 | 2 | 6.18 | 0.06 | 2 | 6.33 | −0.15 |
Ni | I | 5.76 | −0.03 | 0.17 | 25 | 6.28 | 0.16 | 24 | 6.25 | +0.03 |
Sc | II | 2.81 | −0.01 | 0.14 | 5 | 3.31 | 0.08 | 4 | 3.17 | +0.14 |
Si | I | 7.04 | −0.01 | 0.10 | 7 | 7.54 | 0.09 | 7 | 7.55 | −0.01 |
Ti | I | 4.57 | +0.10 | 0.18 | 17 | 4.96 | 0.09 | 12 | 5.02 | −0.06 |
V | I | 3.42 | −0.06 | 0.15 | 8 | 3.97 | 0.19 | 7 | 4.00 | −0.03 |
Y | II | 1.86 | −0.32 | – | 1 | 2.67 | – | 1 | 2.24 | +0.43 |
Zn | I | 4.40 | +0.38 | – | 1 | 4.51 | – | 1 | 4.60 | −0.09 |
Notes. The Gaussian dispersion (σ) around the mean and the number of lines used are also reported. The standard deviation of the mean can be obtained as σ/. The last two columns report the GS98 solar values and the difference with respect to our measurements.
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