Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.54-0.2 | +-0.2 | 2.09 |
CH | ... | -2.29+-0.25 | 0.25+-0.25 | 6.25 |
NH | ... | <-1.47 | <1.07 | <6.5 |
O I | ... | -2.10+-0.21 | 0.44+-0.21 | 6.59 |
Mg I | ... | -2.16+-0.22 | 0.38+-0.22 | 5.45 |
Al I | ... | -3.28+-0.31 | -0.74+-0.31 | 3.17 |
Si I | ... | <-1.68 | <0.86 | <5.87 |
Ca I | ... | -2.07+-0.22 | 0.47+-0.22 | 4.27 |
Sc II | ... | -2.43+-0.15 | 0.11+-0.15 | 0.84 |
Ti I | ... | -2.14+-0.2 | 0.4+-0.2 | 2.81 |
Ti II | ... | -2.10+-0.14 | 0.44+-0.14 | 2.96 |
V II | ... | -2.05+-0.29 | 0.49+-0.29 | 2 |
Cr I | ... | -2.63+-0.21 | -0.09+-0.21 | 3.01 |
Cr II | ... | -2.31+-0.15 | 0.23+-0.15 | 3.45 |
Mn I | ... | -2.69+-0.21 | -0.15+-0.21 | 2.74 |
Mn II | ... | -2.67+-0.21 | -0.13+-0.21 | 2.88 |
Fe I | ... | -2.54+-0.21 | ... | 4.96 |
Fe II | ... | -2.42+-0.14 | ... | 5.08 |
Co I | ... | -2.49+-0.23 | 0.05+-0.23 | 2.51 |
Ni I | ... | -2.38+-0.27 | 0.16+-0.27 | 3.84 |
Zn I | ... | <-2.16 | <0.38 | <2.44 |
Rb I | ... | <-0.12 | <2.42 | <2.48 |
Sr II | ... | -2.25+-0.24 | 0.29+-0.24 | 0.74 |
Y II | ... | -2.80+-0.22 | -0.26+-0.22 | -0.47 |
Zr II | ... | -2.12+-0.17 | 0.42+-0.17 | 0.58 |
Nb II | ... | <0.00 | <2.54 | <1.42 |
Mo I | ... | <-0.88 | <1.66 | <1.04 |
Tc I | ... | <1.36 | <3.90 | <1.36 |
Ba II | ... | -3.02+-0.15 | -0.48+-0.15 | -0.72 |
Ce II | ... | <-1.50 | <1.04 | <0.08 |
Pr II | ... | <-1.07 | <1.47 | <-0.36 |
Nd II | ... | <-1.77 | <0.77 | <-0.27 |
Sm II | ... | <-1.02 | <1.52 | <-0.01 |
Eu II | ... | <-1.86 | <0.68 | <-1.35 |
Gd II | ... | <-0.93 | <1.61 | <0.19 |
Tb II | ... | <-0.19 | <2.35 | <-0.29 |
Dy II | ... | <-1.43 | <1.11 | <-0.29 |
Ho II | ... | <-0.90 | <1.64 | <-0.64 |
Er II | ... | <-1.04 | <1.50 | <-0.11 |
Tm II | ... | <-0.57 | <1.97 | <-0.57 |
Yb II | ... | <-2.25 | <0.29 | <-1.17 |
Hf II | ... | <-0.54 | <2.00 | <0.34 |
Pb I | ... | <-0.41 | <2.13 | <1.54 |
Th II | ... | <-0.35 | <2.19 | <-0.35 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)