Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.97-0.2 | +-0.2 | 1.82 |
CH | ... | -2.40+-0.25 | 0.57+-0.25 | 5.91 |
CN | ... | <-0.17 | <2.80 | <7.8 |
Mg I | ... | -2.48+-0.21 | 0.49+-0.21 | 5.12 |
Al I | ... | -3.75+-0.24 | -0.78+-0.24 | 2.7 |
Si I | ... | -2.36+-0.36 | 0.61+-0.36 | 5.15 |
Ca I | ... | -2.53+-0.23 | 0.44+-0.23 | 3.8 |
Sc II | ... | -2.92+-0.16 | 0.05+-0.16 | 0.1 |
Ti I | ... | -2.52+-0.21 | 0.45+-0.21 | 2.42 |
Ti II | ... | -2.69+-0.14 | 0.28+-0.14 | 2.13 |
Cr I | ... | -3.22+-0.2 | -0.25+-0.2 | 2.42 |
Mn I | ... | -3.49+-0.2 | -0.52+-0.2 | 1.94 |
Fe I | ... | -2.97+-0.21 | ... | 4.53 |
Fe II | ... | -3.1+-0.15 | ... | 4.4 |
Co I | ... | -2.79+-0.23 | 0.18+-0.23 | 2.2 |
Ni I | ... | -3.04+-0.23 | -0.07+-0.23 | 3.18 |
Zn I | ... | <-2.27 | <0.70 | <2.33 |
Sr II | ... | -2.98+-0.17 | -0.01+-0.17 | -0.25 |
Y II | ... | <-2.00 | <0.97 | <0.24 |
Zr II | ... | <-2.34 | <0.63 | <0.26 |
Mo I | ... | <-0.87 | <2.10 | <1.05 |
Tc I | ... | <1.28 | <4.25 | <1.28 |
Ba II | ... | -3.59+-0.15 | -0.62+-0.15 | -1.54 |
Ce II | ... | <-1.71 | <1.26 | <-0.13 |
Pr II | ... | <-1.15 | <1.82 | <-0.44 |
Nd II | ... | <-1.70 | <1.27 | <-0.2 |
Sm II | ... | <-1.14 | <1.83 | <-0.13 |
Eu II | ... | <-1.83 | <1.14 | <-1.32 |
Gd II | ... | <-0.99 | <1.98 | <0.13 |
Tb II | ... | <-0.19 | <2.78 | <-0.29 |
Dy II | ... | <-1.63 | <1.34 | <-0.49 |
Ho II | ... | <-0.86 | <2.11 | <-0.6 |
Er II | ... | <-1.16 | <1.81 | <-0.23 |
Tm II | ... | <-0.61 | <2.36 | <-0.61 |
Hf II | ... | <-0.43 | <2.54 | <0.45 |
Pb I | ... | <-0.52 | <2.45 | <1.43 |
Th II | ... | <-0.34 | <2.63 | <-0.34 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)