Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.29-0.1 | +-0.1 | 1.8 |
CH | ... | -2.41+-0.25 | -0.12+-0.25 | 6.02 |
Mg I | ... | -1.99+-0.15 | 0.3+-0.15 | 5.61 |
Si I | ... | -1.64+-0.23 | 0.65+-0.23 | 5.87 |
Ca I | ... | -1.98+-0.15 | 0.31+-0.15 | 4.36 |
Sc II | ... | -2.45+-0.13 | -0.16+-0.13 | 0.7 |
Ti I | ... | -2.17+-0.1 | 0.12+-0.1 | 2.78 |
Ti II | ... | -2.03+-0.12 | 0.26+-0.12 | 2.92 |
V I | ... | -2.49+-0.18 | -0.2+-0.18 | 1.44 |
Cr I | ... | -2.44+-0.1 | -0.15+-0.1 | 3.2 |
Mn I | ... | -2.66+-0.12 | -0.37+-0.12 | 2.77 |
Fe I | ... | -2.29+-0.1 | ... | 5.21 |
Fe II | ... | -2.29+-0.13 | ... | 5.21 |
Co I | ... | -2.46+-0.2 | -0.17+-0.2 | 2.53 |
Ni I | ... | -2.17+-0.16 | 0.12+-0.16 | 4.05 |
Cu I | ... | -2.62+-0.2 | -0.33+-0.2 | 1.57 |
Zn I | ... | -2.12+-0.12 | 0.17+-0.12 | 2.44 |
Sr II | ... | -1.83+-0.12 | 0.46+-0.12 | 1.04 |
Y II | ... | -2.08+-0.15 | 0.21+-0.15 | 0.13 |
Zr II | ... | -1.88+-0.22 | 0.41+-0.22 | 0.7 |
Ba II | ... | -2.02+-0.12 | 0.27+-0.12 | 0.16 |
Ce II | ... | <-1.54 | <0.75 | <0.04 |
Pr II | ... | <-0.89 | <1.40 | <-0.18 |
Sm II | ... | <-0.87 | <1.42 | <0.14 |
Eu II | ... | -1.73+-0.33 | 0.56+-0.33 | -1.21 |
Gd II | ... | <-0.55 | <1.74 | <0.57 |
Tb II | ... | <0.47 | <2.76 | <0.37 |
Dy II | ... | <-0.89 | <1.40 | <0.25 |
Hf II | ... | <-0.05 | <2.24 | <0.83 |
Pb I | ... | <-0.11 | <2.18 | <1.84 |
Th II | ... | <0.01 | <2.30 | <0.01 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)