Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.62-0.2 | +-0.2 | 2 |
CH | ... | -2.56+-0.25 | 0.06+-0.25 | 6 |
NH | ... | <-2.37 | <0.25 | <5.6 |
Mg I | ... | -2.39+-0.22 | 0.23+-0.22 | 5.22 |
Al I | ... | -3.61+-0.26 | -0.99+-0.26 | 2.84 |
Si I | ... | -2.27+-0.36 | 0.35+-0.36 | 5.24 |
Ca I | ... | -2.25+-0.22 | 0.37+-0.22 | 4.09 |
Sc II | ... | -2.82+-0.15 | -0.2+-0.15 | 0.48 |
Ti I | ... | -2.29+-0.21 | 0.33+-0.21 | 2.66 |
Ti II | ... | -2.35+-0.15 | 0.27+-0.15 | 2.74 |
V I | ... | -2.31+-0.25 | 0.31+-0.25 | 1.62 |
V II | ... | -2.61+-0.33 | 0.01+-0.33 | 1.46 |
Cr I | ... | -2.78+-0.21 | -0.16+-0.21 | 2.87 |
Cr II | ... | -2.31+-0.15 | 0.31+-0.15 | 3.48 |
Mn I | ... | -2.86+-0.21 | -0.24+-0.21 | 2.57 |
Mn II | ... | -2.93+-0.22 | -0.31+-0.22 | 2.65 |
Fe I | ... | -2.62+-0.21 | ... | 4.88 |
Fe II | ... | -2.47+-0.15 | ... | 5.03 |
Co I | ... | -2.68+-0.25 | -0.06+-0.25 | 2.31 |
Ni I | ... | -2.65+-0.27 | -0.03+-0.27 | 3.57 |
Sr II | ... | -2.68+-0.23 | -0.06+-0.23 | 0.34 |
Y II | ... | -2.83+-0.17 | -0.21+-0.17 | -0.47 |
Zr II | ... | -2.73+-0.25 | -0.11+-0.25 | -0.13+-0.25 |
Nb II | ... | <-0.11 | <2.51 | <1.31 |
Mo I | ... | <-1.02 | <1.60 | <0.9 |
Tc I | ... | <1.30 | <3.92 | <1.3 |
Ba II | ... | -3.39+-0.14 | -0.77+-0.14 | -1.06 |
Ce II | ... | <-1.65 | <0.97 | <-0.07 |
Pr II | ... | <-1.12 | <1.50 | <-0.41 |
Nd II | ... | <-1.82 | <0.80 | <-0.32 |
Sm II | ... | <-1.22 | <1.40 | <-0.21 |
Eu II | ... | <-1.85 | <0.77 | <-1.34 |
Gd II | ... | <-0.96 | <1.66 | <0.16 |
Tb II | ... | <-0.26 | <2.36 | <-0.36 |
Dy II | ... | <-1.50 | <1.12 | <-0.36 |
Er II | ... | <-1.28 | <1.34 | <-0.35 |
Tm II | ... | <-0.67 | <1.95 | <-0.67 |
Yb II | ... | <-2.33 | <0.29 | <-1.25 |
Hf II | ... | <-0.39 | <2.23 | <0.49 |
Pb I | ... | <-0.40 | <2.22 | <1.55 |
Th II | ... | <-0.44 | <2.18 | <-0.44 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)