Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.35 | <3.24 | <1.51 |
CH | ... | -1.11+-0.25 | 1.78+-0.25 | 7.48 |
CN | ... | -0.84+-0.28 | 2.05+-0.28 | 7.15 |
O I | ... | -2.11+-0.2 | 0.78+-0.2 | 6.58 |
Mg I | ... | -2.46+-0.22 | 0.43+-0.22 | 5.13 |
Al I | ... | -3.48+-0.27 | -0.59+-0.27 | 2.97 |
K I | ... | <-2.46 | <0.43 | <2.66 |
Ca I | ... | -2.48+-0.22 | 0.41+-0.22 | 3.86 |
Sc II | ... | -3.03+-0.14 | -0.14+-0.14 | 0.28 |
Ti I | ... | -2.58+-0.23 | 0.31+-0.23 | 2.37 |
Ti II | ... | -2.76+-0.14 | 0.13+-0.14 | 2.34 |
V II | ... | <-2.11 | <0.78 | <1.89 |
Cr I | ... | -3.12+-0.2 | -0.23+-0.2 | 2.52 |
Mn I | ... | -3.36+-0.2 | -0.47+-0.2 | 2.07 |
Fe I | ... | -2.89+-0.21 | ... | 4.61 |
Fe II | ... | -2.73+-0.15 | ... | 4.77 |
Co I | ... | -2.79+-0.24 | 0.1+-0.24 | 2.19 |
Cu I | ... | <-1.66 | <1.23 | <2.55 |
Zn I | ... | <-1.95 | <0.94 | <2.65 |
Rb I | ... | <0.11 | <3.00 | <2.71 |
Sr II | ... | -2.50+-0.24 | 0.39+-0.24 | 0.52 |
Y II | ... | -2.82+-0.19 | 0.07+-0.19 | -0.45 |
Nb II | ... | <0.32 | <3.21 | <1.74 |
Mo I | ... | <-0.48 | <2.41 | <1.44 |
Tc I | ... | <1.92 | <4.81 | <1.92 |
Ba II | ... | -2.40+-0.14 | 0.49+-0.14 | -0.07 |
La II | ... | <-1.64 | <1.25 | <-0.47 |
Ce II | ... | <-1.30 | <1.59 | <0.28 |
Pr II | ... | <-0.82 | <2.07 | <-0.11 |
Nd II | ... | <-1.43 | <1.46 | <0.07 |
Sm II | ... | <-0.82 | <2.07 | <0.19 |
Eu II | ... | -1.76+-0.19 | 1.13+-0.19 | -1.08 |
Gd II | ... | <-0.62 | <2.27 | <0.5 |
Tb II | ... | <0.10 | <2.99 | <0 |
Dy II | ... | <-1.36 | <1.53 | <-0.22 |
Ho II | ... | <-0.43 | <2.46 | <-0.17 |
Er II | ... | <-0.87 | <2.02 | <0.06 |
Tm II | ... | <0.43 | <3.32 | <0.43 |
Yb II | ... | -1.87+-0.18 | 1.02+-0.18 | -0.79 |
Hf II | ... | <-0.15 | <2.74 | <0.73 |
Pb I | ... | <0.14 | <3.03 | <2.09 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)