Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.84-0.14 | +-0.14 | 1.24 |
CH | ... | -2.67+-0.25 | 0.17+-0.25 | 5.76 |
NH | ... | <-2.17 | <0.67 | <5.8 |
O I | ... | <-2.24 | <0.60 | <6.63 |
Mg I | ... | -2.36+-0.15 | 0.48+-0.15 | 5.24 |
Al I | ... | -3.47+-0.3 | -0.63+-0.3 | 2.98 |
Si I | ... | -1.99+-0.28 | 0.85+-0.28 | 5.52 |
K I | ... | -2.58+-0.19 | 0.26+-0.19 | 2.45 |
Ca I | ... | -2.37+-0.17 | 0.47+-0.17 | 3.97 |
Sc II | ... | -2.85+-0.15 | -0.01+-0.15 | 0.31 |
Ti I | ... | -2.58+-0.14 | 0.26+-0.14 | 2.37 |
Ti II | ... | -2.59+-0.15 | 0.25+-0.15 | 2.37 |
V I | ... | -3.31+-0.21 | -0.47+-0.21 | 0.62 |
V II | ... | -2.91+-0.28 | -0.07+-0.28 | 1.03 |
Cr I | ... | -3.09+-0.15 | -0.25+-0.15 | 2.54 |
Cr II | ... | -2.57+-0.16 | 0.27+-0.16 | 3.08 |
Mn I | ... | -3.06+-0.24 | -0.22+-0.24 | 2.36 |
Mn II | ... | -3.28+-0.21 | -0.44+-0.21 | 2.15 |
Fe I | ... | -2.84+-0.14 | ... | 4.66 |
Fe II | ... | -2.83+-0.15 | ... | 4.67 |
Co I | ... | -2.83+-0.21 | 0.01+-0.21 | 2.16 |
Ni I | ... | -2.65+-0.21 | 0.19+-0.21 | 3.57 |
Zn I | ... | -2.62+-0.16 | 0.22+-0.16 | 1.94 |
Rb I | ... | <-0.55 | <2.29 | <2.05 |
Sr II | ... | -2.72+-0.25 | 0.12+-0.25 | 0.16 |
Y II | ... | -3.29+-0.18 | -0.45+-0.18 | -1.07 |
Zr II | ... | -2.80+-0.19 | 0.04+-0.19 | -0.22 |
Nb II | ... | <-0.63 | <2.21 | <0.79 |
Mo I | ... | <-1.67 | <1.17 | <0.25 |
Sn I | ... | <-0.33 | <2.51 | <1.67 |
Ba II | ... | -3.57+-0.15 | -0.73+-0.15 | -1.39 |
La II | ... | <-2.49 | <0.35 | <-1.32 |
Ce II | ... | <-2.45 | <0.39 | <-0.87 |
Pr II | ... | <-1.77 | <1.07 | <-1.06 |
Nd II | ... | <-2.62 | <0.22 | <-1.12 |
Sm II | ... | <-2.06 | <0.78 | <-1.05 |
Eu II | ... | -2.51+-0.18 | 0.33+-0.18 | -1.99 |
Gd II | ... | <-1.53 | <1.31 | <-0.41 |
Tb II | ... | <-1.03 | <1.81 | <-1.13 |
Dy II | ... | <-2.52 | <0.32 | <-1.38 |
Er II | ... | <-1.92 | <0.92 | <-0.99 |
Tm II | ... | <-1.19 | <1.65 | <-1.19 |
Yb II | ... | -2.91+-0.23 | -0.07+-0.23 | -1.98 |
Hf II | ... | <-1.19 | <1.65 | <-0.31 |
Pb I | ... | <-1.05 | <1.79 | <0.9 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)