Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.93-0.2 | +-0.2 | 1.93 |
CH | ... | -2.45+-0.25 | 0.48+-0.25 | 6 |
NH | ... | <-2.22 | <0.71 | <5.75 |
O I | ... | <-2.31 | <0.62 | <6.56 |
Mg I | ... | -2.43+-0.22 | 0.5+-0.22 | 5.17 |
Al I | ... | -3.69+-0.29 | -0.76+-0.29 | 2.76 |
Si I | ... | -2.03+-0.37 | 0.9+-0.37 | 5.48 |
Ca I | ... | -2.38+-0.22 | 0.55+-0.22 | 3.96 |
Sc II | ... | -2.94+-0.15 | -0.01+-0.15 | 0.23 |
Ti I | ... | -2.63+-0.21 | 0.3+-0.21 | 2.33 |
Ti II | ... | -2.71+-0.14 | 0.22+-0.14 | 2.26 |
V II | ... | <-2.11 | <0.82 | <1.89 |
Cr I | ... | -3.17+-0.21 | -0.24+-0.21 | 2.47 |
Cr II | ... | -2.59+-0.17 | 0.34+-0.17 | 3.07 |
Mn I | ... | -3.41+-0.2 | -0.48+-0.2 | 2.02 |
Mn II | ... | -3.24+-0.2 | -0.31+-0.2 | 2.21 |
Fe I | ... | -2.93+-0.21 | ... | 4.57 |
Fe II | ... | -2.91+-0.15 | ... | 4.59 |
Co I | ... | -2.79+-0.23 | 0.14+-0.23 | 2.2 |
Ni I | ... | -2.86+-0.28 | 0.07+-0.28 | 3.37 |
Zn I | ... | <-2.17 | <0.76 | <2.43 |
Rb I | ... | <0.22 | <3.15 | <2.82 |
Sr II | ... | -2.72+-0.24 | 0.21+-0.24 | 0.16 |
Y II | ... | -3.22+-0.2 | -0.29+-0.2 | -1 |
Zr II | ... | -2.35+-0.2 | 0.58+-0.2 | 0.25 |
Nb II | ... | <-0.04 | <2.89 | <1.38 |
Mo I | ... | <-0.98 | <1.95 | <0.94 |
Tc I | ... | <1.38 | <4.31 | <1.38 |
Ba II | ... | -3.54+-0.14 | -0.61+-0.14 | -1.34 |
La II | ... | <-2.00 | <0.93 | <-0.83 |
Ce II | ... | <-1.69 | <1.24 | <-0.11 |
Pr II | ... | <-1.33 | <1.60 | <-0.62 |
Nd II | ... | <-1.63 | <1.30 | <-0.13 |
Sm II | ... | <-1.19 | <1.74 | <-0.18 |
Eu II | ... | <-1.96 | <0.97 | <-1.45 |
Gd II | ... | <-1.02 | <1.91 | <0.1 |
Tb II | ... | <-0.29 | <2.64 | <-0.39 |
Dy II | ... | <-1.74 | <1.19 | <-0.6 |
Ho II | ... | <-0.94 | <1.99 | <-0.68 |
Er II | ... | <-1.17 | <1.76 | <-0.24 |
Tm II | ... | <-0.83 | <2.10 | <-0.83 |
Yb II | ... | <-2.49 | <0.44 | <-1.41 |
Hf II | ... | <-0.48 | <2.45 | <0.4 |
Pb I | ... | <-0.35 | <2.58 | <1.6 |
Th II | ... | <-0.68 | <2.25 | <-0.68 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)