Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.33-0.1 | +-0.1 | 1.59 |
CH | ... | -2.58+-0.25 | -0.25+-0.25 | 5.85 |
Mg I | ... | -1.97+-0.15 | 0.36+-0.15 | 5.62 |
Ca I | ... | -1.95+-0.15 | 0.38+-0.15 | 4.38 |
Sc II | ... | -2.46+-0.13 | -0.13+-0.13 | 0.69 |
Ti I | ... | -2.13+-0.1 | 0.2+-0.1 | 2.82 |
Ti II | ... | -2.01+-0.13 | 0.32+-0.13 | 2.94 |
V I | ... | -2.42+-0.18 | -0.09+-0.18 | 1.51 |
Cr I | ... | -2.41+-0.1 | -0.08+-0.1 | 3.22 |
Mn I | ... | -2.76+-0.13 | -0.43+-0.13 | 2.66 |
Fe I | ... | -2.33+-0.1 | ... | 5.17 |
Fe II | ... | -2.33+-0.14 | ... | 5.17 |
Co I | ... | -2.38+-0.21 | -0.05+-0.21 | 2.61 |
Ni I | ... | -2.18+-0.16 | 0.15+-0.16 | 4.03 |
Zn I | ... | -2.25+-0.15 | 0.08+-0.15 | 2.31 |
Sr II | ... | -2.33+-0.15 | 0.00+-0.15 | 0.54 |
Y II | ... | <-2.72 | <-0.39 | <-0.48 |
Zr II | ... | <-1.73 | <0.60 | <0.87 |
Ba II | ... | -2.63+-0.12 | -0.3+-0.12 | -0.44 |
La II | ... | <-1.75 | <0.58 | <-0.58 |
Ce II | ... | <-1.47 | <0.86 | <0.11 |
Pr II | ... | <-1.00 | <1.33 | <-0.29 |
Nd II | ... | <-1.39 | <0.94 | <0.11 |
Sm II | ... | <-1.14 | <1.19 | <-0.13 |
Eu II | ... | <-1.63 | <0.70 | <-1.12 |
Gd II | ... | <-0.67 | <1.66 | <0.45 |
Tb II | ... | <0.29 | <2.62 | <0.19 |
Dy II | ... | <-1.05 | <1.28 | <0.09 |
Tm II | ... | <0.80 | <3.13 | <0.8 |
Hf II | ... | <-0.18 | <2.15 | <0.7 |
Pb I | ... | <-0.49 | <1.84 | <1.46 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)