Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.33 | <3.25 | <1.49 |
CH | ... | -2.43+-0.25 | 0.49+-0.25 | 6.05 |
NH | ... | <-1.27 | <1.65 | <6.7 |
O I | ... | -2.38+-0.22 | 0.54+-0.22 | 6.31 |
Mg I | ... | -2.38+-0.22 | 0.54+-0.22 | 5.22 |
Al I | ... | -3.58+-0.25 | -0.66+-0.25 | 2.87 |
Si I | ... | -2.32+-0.36 | 0.6+-0.36 | 5.19 |
Ca I | ... | -2.44+-0.22 | 0.48+-0.22 | 3.9 |
Sc II | ... | -3.05+-0.16 | -0.13+-0.16 | 0.15 |
Ti I | ... | -2.58+-0.21 | 0.34+-0.21 | 2.37 |
Ti II | ... | -2.77+-0.14 | 0.15+-0.14 | 2.23 |
V II | ... | -2.17+-0.26 | 0.75+-0.26 | 1.81 |
Cr I | ... | -3.17+-0.2 | -0.25+-0.2 | 2.47 |
Mn I | ... | -3.40+-0.2 | -0.48+-0.2 | 2.03 |
Mn II | ... | -3.32+-0.21 | -0.4+-0.21 | 2.16 |
Fe I | ... | -2.92+-0.21 | ... | 4.58 |
Fe II | ... | -2.87+-0.15 | ... | 4.63 |
Co I | ... | -2.88+-0.24 | 0.04+-0.24 | 2.11 |
Ni I | ... | -2.84+-0.28 | 0.08+-0.28 | 3.38 |
Zn I | ... | -2.16+-0.21 | 0.76+-0.21 | 2.4 |
Rb I | ... | <0.06 | <2.98 | <2.66 |
Sr II | ... | -3.29+-0.17 | -0.37+-0.17 | -0.37 |
Y II | ... | <-3.12 | <-0.20 | <-0.88 |
Zr II | ... | <-2.34 | <0.58 | <0.26 |
Nb II | ... | <0.04 | <2.96 | <1.46 |
Mo I | ... | <-0.68 | <2.24 | <1.24 |
Tc I | ... | <1.51 | <4.43 | <1.51 |
Ba II | ... | -3.49+-0.14 | -0.57+-0.14 | -1.26 |
Ce II | ... | <-1.54 | <1.38 | <0.04 |
Pr II | ... | <-0.94 | <1.98 | <-0.23 |
Nd II | ... | <-1.55 | <1.37 | <-0.05 |
Sm II | ... | <-1.06 | <1.86 | <-0.05 |
Eu II | ... | <-1.73 | <1.19 | <-1.22 |
Gd II | ... | <-0.91 | <2.01 | <0.21 |
Tb II | ... | <-0.28 | <2.64 | <-0.38 |
Dy II | ... | <-1.40 | <1.52 | <-0.26 |
Ho II | ... | <-0.77 | <2.15 | <-0.51 |
Er II | ... | <-1.10 | <1.82 | <-0.17 |
Tm II | ... | <-0.65 | <2.27 | <-0.65 |
Yb II | ... | <-2.12 | <0.80 | <-1.04 |
Hf II | ... | <-0.25 | <2.67 | <0.63 |
Pb I | ... | <-0.47 | <2.45 | <1.48 |
Th II | ... | <-0.18 | <2.74 | <-0.18 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)