Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.12-0.2 | +-0.2 | 2.05 |
CH | ... | <-2.40 | <0.72 | <6.15 |
NH | ... | <-1.67 | <1.45 | <6.3 |
Mg I | ... | -2.70+-0.22 | 0.42+-0.22 | 4.9 |
Al I | ... | -3.87+-0.22 | -0.75+-0.22 | 2.58 |
Si I | ... | -2.62+-0.36 | 0.5+-0.36 | 4.89 |
Ca I | ... | -2.75+-0.23 | 0.37+-0.23 | 3.59 |
Sc II | ... | -3.04+-0.15 | 0.08+-0.15 | 0.02 |
Ti I | ... | -2.22+-0.22 | 0.9+-0.22 | 2.73 |
Ti II | ... | -2.85+-0.14 | 0.27+-0.14 | 2.02 |
V II | ... | <-2.16 | <0.96 | <1.84 |
Cr I | ... | -3.35+-0.2 | -0.23+-0.2 | 2.29 |
Mn I | ... | -3.67+-0.22 | -0.55+-0.22 | 1.76 |
Fe I | ... | -3.12+-0.21 | ... | 4.38 |
Fe II | ... | -3.2+-0.15 | ... | 4.3 |
Co I | ... | -2.93+-0.23 | 0.19+-0.23 | 2.06 |
Ni I | ... | -3.07+-0.23 | 0.05+-0.23 | 3.15 |
Zn I | ... | <-1.97 | <1.15 | <2.63 |
Ga I | ... | <-1.15 | <1.97 | <1.73 |
Sr II | ... | -3.27+-0.14 | -0.15+-0.14 | -0.48 |
Y II | ... | <-2.20 | <0.92 | <0.04 |
Zr II | ... | <-2.13 | <0.99 | <0.47 |
Nb II | ... | <0.24 | <3.36 | <1.66 |
Mo I | ... | <-0.62 | <2.50 | <1.3 |
Tc I | ... | <1.50 | <4.62 | <1.5 |
Ba II | ... | -3.63+-0.16 | -0.51+-0.16 | -1.53 |
Ce II | ... | <-1.53 | <1.59 | <0.05 |
Pr II | ... | <-0.86 | <2.26 | <-0.15 |
Nd II | ... | <-1.52 | <1.60 | <-0.02 |
Sm II | ... | <-1.03 | <2.09 | <-0.02 |
Eu II | ... | <-1.71 | <1.41 | <-1.2 |
Gd II | ... | <-0.83 | <2.29 | <0.29 |
Tb II | ... | <-0.03 | <3.09 | <-0.13 |
Dy II | ... | <-1.49 | <1.63 | <-0.35 |
Ho II | ... | <-0.78 | <2.34 | <-0.52 |
Er II | ... | <-1.03 | <2.09 | <-0.1 |
Tm II | ... | <0.51 | <3.63 | <0.51 |
Yb II | ... | <-1.96 | <1.16 | <-0.88 |
Hf II | ... | <-0.16 | <2.96 | <0.72 |
Pb I | ... | <-0.22 | <2.90 | <1.73 |
Th II | ... | <-0.39 | <2.73 | <-0.39 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)