Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.73-0.2 | +-0.2 | 2.04 |
CH | ... | -2.57+-0.25 | 0.16+-0.25 | 6.07 |
NH | ... | <-1.52 | <1.21 | <6.45 |
O I | ... | <-2.31 | <0.42 | <6.56 |
Na I | ... | -2.94+-0.27 | -0.21+-0.27 | 3.3 |
Mg I | ... | -2.35+-0.22 | 0.38+-0.22 | 5.25 |
Al I | ... | -3.44+-0.28 | -0.71+-0.28 | 3.01 |
Si I | ... | -2.31+-0.36 | 0.42+-0.36 | 5.2 |
Ca I | ... | -2.19+-0.22 | 0.54+-0.22 | 4.15 |
Sc II | ... | -2.58+-0.15 | 0.15+-0.15 | 0.79 |
Ti I | ... | -2.27+-0.21 | 0.46+-0.21 | 2.68 |
Ti II | ... | -2.38+-0.14 | 0.35+-0.14 | 2.79 |
Cr I | ... | -2.85+-0.21 | -0.12+-0.21 | 2.78 |
Cr II | ... | -2.42+-0.15 | 0.31+-0.15 | 3.44 |
Mn I | ... | -3.15+-0.2 | -0.42+-0.2 | 2.28 |
Mn II | ... | -3.08+-0.29 | -0.35+-0.29 | 2.57 |
Fe I | ... | -2.73+-0.21 | ... | 4.77 |
Fe II | ... | -2.51+-0.15 | ... | 4.99 |
Co I | ... | -2.60+-0.23 | 0.13+-0.23 | 2.39 |
Ni I | ... | -2.70+-0.28 | 0.03+-0.28 | 3.52 |
Zn I | ... | <-2.16 | <0.57 | <2.44 |
Rb I | ... | <0.23 | <2.96 | <2.83 |
Sr II | ... | -2.58+-0.24 | 0.15+-0.24 | 0.51 |
Y II | ... | <-2.89 | <-0.16 | <-0.65 |
Zr II | ... | -2.48+-0.2 | 0.25+-0.2 | 0.32 |
Nb II | ... | <-0.12 | <2.61 | <1.3 |
Mo I | ... | <-0.50 | <2.23 | <1.42 |
Tc I | ... | <1.47 | <4.20 | <1.47 |
Ba II | ... | -3.39+-0.14 | -0.66+-0.14 | -0.99 |
Ce II | ... | <-1.51 | <1.22 | <0.07 |
Pr II | ... | <-0.79 | <1.94 | <-0.08 |
Nd II | ... | <-1.57 | <1.16 | <-0.07 |
Sm II | ... | <-0.94 | <1.79 | <0.07 |
Eu II | ... | <-1.78 | <0.95 | <-1.27 |
Gd II | ... | <-0.78 | <1.95 | <0.34 |
Tb II | ... | <-0.12 | <2.61 | <-0.22 |
Dy II | ... | <-1.34 | <1.39 | <-0.2 |
Ho II | ... | <-0.79 | <1.94 | <-0.53 |
Er II | ... | <-1.00 | <1.73 | <-0.07 |
Tm II | ... | <-0.53 | <2.20 | <-0.53 |
Yb II | ... | <-2.33 | <0.40 | <-1.25 |
Hf II | ... | <-0.19 | <2.54 | <0.69 |
Pb I | ... | <-0.24 | <2.49 | <1.71 |
Th II | ... | <-0.21 | <2.52 | <-0.21 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)