Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.14-0.2 | +-0.2 | 2.05 |
CH | ... | <-2.55 | <0.59 | <6 |
NH | ... | <-1.57 | <1.57 | <6.4 |
Mg I | ... | -2.71+-0.23 | 0.43+-0.23 | 4.9 |
Al I | ... | -3.87+-0.22 | -0.73+-0.22 | 2.58 |
Si I | ... | -2.73+-0.36 | 0.41+-0.36 | 4.78 |
Ca I | ... | -2.56+-0.22 | 0.58+-0.22 | 3.78 |
Sc II | ... | -3.14+-0.16 | 0.00+-0.16 | 0.34 |
Ti I | ... | -2.47+-0.21 | 0.67+-0.21 | 2.48 |
Ti II | ... | -2.85+-0.14 | 0.29+-0.14 | 2.43 |
V II | ... | <-2.42 | <0.72 | <1.58 |
Cr I | ... | -3.30+-0.2 | -0.16+-0.2 | 2.35 |
Cr II | ... | -3.03+-0.19 | 0.11+-0.19 | 2.93 |
Mn I | ... | -3.57+-0.21 | -0.43+-0.21 | 1.86 |
Mn II | ... | -3.62+-0.21 | -0.48+-0.21 | 2.13 |
Fe I | ... | -3.14+-0.21 | ... | 4.36 |
Fe II | ... | -2.82+-0.14 | ... | 4.68 |
Co I | ... | -2.97+-0.25 | 0.17+-0.25 | 2.02 |
Ni I | ... | -3.11+-0.25 | 0.03+-0.25 | 3.11 |
Sr II | ... | -3.56+-0.17 | -0.42+-0.17 | -0.37 |
Y II | ... | <-3.39 | <-0.25 | <-1.15 |
Zr II | ... | <-2.25 | <0.89 | <0.35 |
Nb II | ... | <-0.09 | <3.05 | <1.33 |
Mo I | ... | <-1.00 | <2.14 | <0.92 |
Tc I | ... | <1.26 | <4.40 | <1.26 |
Ba II | ... | -3.85+-0.15 | -0.71+-0.15 | -1.35 |
Ce II | ... | <-1.54 | <1.60 | <0.04 |
Pr II | ... | <-1.08 | <2.06 | <-0.37 |
Nd II | ... | <-1.76 | <1.38 | <-0.26 |
Sm II | ... | <-1.09 | <2.05 | <-0.08 |
Eu II | ... | <-1.89 | <1.25 | <-1.38 |
Gd II | ... | <-1.09 | <2.05 | <0.03 |
Tb II | ... | <-0.31 | <2.83 | <-0.41 |
Dy II | ... | <-1.61 | <1.53 | <-0.47 |
Ho II | ... | <-0.98 | <2.16 | <-0.72 |
Er II | ... | <-1.12 | <2.02 | <-0.19 |
Tm II | ... | <-0.77 | <2.37 | <-0.77 |
Yb II | ... | <-2.42 | <0.72 | <-1.34 |
Hf II | ... | <-0.38 | <2.76 | <0.5 |
Pb I | ... | <-0.51 | <2.63 | <1.44 |
Th II | ... | <-0.57 | <2.57 | <-0.57 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)