Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.00-0.2 | +-0.2 | 2.01 |
CH | ... | <-2.40 | <0.60 | <6.15 |
NH | ... | <-1.62 | <1.38 | <6.35 |
O I | ... | <-2.77 | <0.23 | <6.1 |
Mg I | ... | -2.56+-0.22 | 0.44+-0.22 | 5.03 |
Al I | ... | -3.70+-0.23 | -0.7+-0.23 | 2.74 |
Si I | ... | -2.45+-0.36 | 0.55+-0.36 | 5.06 |
Ca I | ... | -2.45+-0.22 | 0.55+-0.22 | 3.89 |
Sc II | ... | -3.06+-0.15 | -0.06+-0.15 | 0.21 |
Ti I | ... | -2.55+-0.22 | 0.45+-0.22 | 2.4 |
Ti II | ... | -2.79+-0.14 | 0.21+-0.14 | 2.28 |
Cr I | ... | -3.17+-0.2 | -0.17+-0.2 | 2.47 |
Mn I | ... | -3.46+-0.21 | -0.46+-0.21 | 1.97 |
Mn II | ... | -3.37+-0.21 | -0.37+-0.21 | 2.18 |
Fe I | ... | -3+-0.22 | ... | 4.5 |
Fe II | ... | -2.88+-0.15 | ... | 4.62 |
Co I | ... | -2.86+-0.25 | 0.14+-0.25 | 2.13 |
Ni I | ... | -3.02+-0.27 | -0.02+-0.27 | 3.2 |
Zn I | ... | <-2.06 | <0.94 | <2.54 |
Rb I | ... | <0.09 | <3.09 | <2.69 |
Sr II | ... | -3.35+-0.16 | -0.35+-0.16 | -0.36 |
Y II | ... | <-2.72 | <0.28 | <-0.48 |
Zr II | ... | <-2.27 | <0.73 | <0.33 |
Nb II | ... | <-0.09 | <2.91 | <1.33 |
Mo I | ... | <-0.70 | <2.30 | <1.22 |
Tc I | ... | <1.39 | <4.39 | <1.39 |
Ba II | ... | -3.51+-0.14 | -0.51+-0.14 | -1.21 |
La II | ... | <-1.88 | <1.12 | <-0.71 |
Ce II | ... | <-1.49 | <1.51 | <0.09 |
Pr II | ... | <-0.57 | <2.43 | <0.14 |
Nd II | ... | <-1.56 | <1.44 | <-0.06 |
Sm II | ... | <-1.01 | <1.99 | <0 |
Eu II | ... | <-1.83 | <1.17 | <-1.32 |
Gd II | ... | <-0.93 | <2.07 | <0.19 |
Tb II | ... | <-0.10 | <2.90 | <-0.2 |
Dy II | ... | <-1.49 | <1.51 | <-0.35 |
Ho II | ... | <-0.82 | <2.18 | <-0.56 |
Er II | ... | <-1.14 | <1.86 | <-0.21 |
Tm II | ... | <-0.55 | <2.45 | <-0.55 |
Yb II | ... | <-2.09 | <0.91 | <-1.01 |
Hf II | ... | <-0.37 | <2.63 | <0.51 |
Pb I | ... | <-0.38 | <2.62 | <1.57 |
Th II | ... | <-0.38 | <2.62 | <-0.38 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)