Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.15-0.2 | +-0.2 | 1.88 |
CH | ... | -3.20+-0.25 | -0.05+-0.25 | 5.57 |
CN | ... | <-0.22 | <2.93 | <7.75 |
O I | ... | <-2.20 | <0.95 | <6.67 |
Mg I | ... | -2.63+-0.21 | 0.52+-0.21 | 4.97 |
Al I | ... | -3.84+-0.24 | -0.69+-0.24 | 2.62 |
Si I | ... | -2.61+-0.36 | 0.54+-0.36 | 4.9 |
Ca I | ... | -2.46+-0.22 | 0.69+-0.22 | 3.88 |
Sc II | ... | -3.23+-0.16 | -0.08+-0.16 | 0.26 |
Ti I | ... | -2.49+-0.2 | 0.66+-0.2 | 2.46 |
Ti II | ... | -2.84+-0.14 | 0.31+-0.14 | 2.45 |
Cr I | ... | -3.35+-0.2 | -0.2+-0.2 | 2.29 |
Cr II | ... | -3.00+-0.18 | 0.15+-0.18 | 2.98 |
Mn I | ... | -3.66+-0.21 | -0.51+-0.21 | 1.78 |
Mn II | ... | -3.83+-0.21 | -0.68+-0.21 | 1.94 |
Fe I | ... | -3.15+-0.21 | ... | 4.35 |
Fe II | ... | -2.81+-0.15 | ... | 4.69 |
Co I | ... | -3.06+-0.24 | 0.09+-0.24 | 1.93 |
Ni I | ... | -3.17+-0.25 | -0.02+-0.25 | 3.06 |
Zn I | ... | <-2.27 | <0.88 | <2.33 |
Rb I | ... | <0.06 | <3.21 | <2.66 |
Sr II | ... | -2.97+-0.23 | 0.18+-0.23 | 0.23 |
Y II | ... | -3.31+-0.2 | -0.16+-0.2 | -0.76 |
Zr II | ... | -2.99+-0.24 | 0.16+-0.24 | -0.07 |
Nb II | ... | <-0.05 | <3.10 | <1.37 |
Mo I | ... | <-0.91 | <2.24 | <1.01 |
Tc I | ... | <1.06 | <4.21 | <1.06 |
Sn I | ... | <0.30 | <3.45 | <2.3 |
Ba II | ... | -3.89+-0.14 | -0.74+-0.14 | -1.37 |
Ce II | ... | <-1.62 | <1.53 | <-0.04 |
Pr II | ... | <-1.21 | <1.94 | <-0.5 |
Nd II | ... | <-1.21 | <1.94 | <0.29 |
Sm II | ... | <-1.20 | <1.95 | <-0.19 |
Eu II | ... | <-2.06 | <1.09 | <-1.55 |
Gd II | ... | <-0.93 | <2.22 | <0.19 |
Tb II | ... | <-0.40 | <2.75 | <-0.5 |
Dy II | ... | <-1.45 | <1.70 | <-0.31 |
Ho II | ... | <-0.87 | <2.28 | <-0.61 |
Er II | ... | <-1.01 | <2.14 | <-0.08 |
Tm II | ... | <-0.78 | <2.37 | <-0.78 |
Yb II | ... | <-2.24 | <0.91 | <-1.16 |
Hf II | ... | <-0.33 | <2.82 | <0.55 |
Pb I | ... | <-0.40 | <2.75 | <1.55 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)