Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.53-0.2 | +-0.2 | 2.17 |
CH | ... | -2.26+-0.25 | 0.27+-0.25 | 6.16 |
NH | ... | <-1.47 | <1.06 | <6.5 |
O I | ... | -2.42+-0.21 | 0.11+-0.21 | 6.27 |
Mg I | ... | -2.28+-0.22 | 0.25+-0.22 | 5.32 |
Al I | ... | -3.36+-0.3 | -0.83+-0.3 | 3.09 |
Si I | ... | -1.97+-0.36 | 0.56+-0.36 | 5.54 |
Ca I | ... | -2.14+-0.22 | 0.39+-0.22 | 4.2 |
Sc II | ... | -2.54+-0.16 | -0.01+-0.16 | 0.6 |
Ti I | ... | -2.17+-0.21 | 0.36+-0.21 | 2.79 |
Ti II | ... | -2.26+-0.15 | 0.27+-0.15 | 2.68 |
V II | ... | -2.37+-0.31 | 0.16+-0.31 | 1.55 |
Cr I | ... | -2.70+-0.21 | -0.17+-0.21 | 2.94 |
Cr II | ... | -2.32+-0.16 | 0.21+-0.16 | 3.32 |
Mn I | ... | -2.72+-0.21 | -0.19+-0.21 | 2.72 |
Mn II | ... | -2.67+-0.21 | -0.14+-0.21 | 2.75 |
Fe I | ... | -2.53+-0.21 | ... | 4.97 |
Fe II | ... | -2.54+-0.15 | ... | 4.96 |
Co I | ... | -2.46+-0.26 | 0.07+-0.26 | 2.54 |
Ni I | ... | -2.48+-0.28 | 0.05+-0.28 | 3.74 |
Zn I | ... | -2.28+-0.24 | 0.25+-0.24 | 2.28 |
Rb I | ... | <0.30 | <2.83 | <2.9 |
Sr II | ... | -2.82+-0.19 | -0.29+-0.19 | 0.04 |
Y II | ... | -2.90+-0.24 | -0.37+-0.24 | -0.69 |
Zr II | ... | -2.36+-0.18 | 0.17+-0.18 | 0.21 |
Nb II | ... | <-0.05 | <2.48 | <1.37 |
Mo I | ... | <-0.93 | <1.60 | <0.99 |
Tc I | ... | <1.49 | <4.02 | <1.49 |
Ba II | ... | -3.03+-0.14 | -0.5+-0.14 | -0.86 |
Ce II | ... | <-1.45 | <1.08 | <0.13 |
Pr II | ... | <-1.00 | <1.53 | <-0.29 |
Nd II | ... | <-1.60 | <0.93 | <-0.1 |
Sm II | ... | <-1.12 | <1.41 | <-0.11 |
Eu II | ... | <-1.78 | <0.75 | <-1.27 |
Gd II | ... | <-0.94 | <1.59 | <0.18 |
Tb II | ... | <-0.31 | <2.22 | <-0.41 |
Dy II | ... | <-1.42 | <1.11 | <-0.28 |
Ho II | ... | <-0.74 | <1.79 | <-0.48 |
Er II | ... | <-1.16 | <1.37 | <-0.23 |
Tm II | ... | <-0.71 | <1.82 | <-0.71 |
Yb II | ... | <-2.41 | <0.12 | <-1.33 |
Hf II | ... | <-0.35 | <2.18 | <0.53 |
Pb I | ... | <-0.33 | <2.20 | <1.62 |
Th II | ... | <-0.41 | <2.12 | <-0.41 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)