Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.09-0.2 | +-0.2 | 1.7 |
CH | ... | <-2.45 | <0.64 | <6.1 |
CN | ... | <0.23 | <3.32 | <8.2 |
Mg I | ... | -2.58+-0.21 | 0.51+-0.21 | 5.01 |
Al I | ... | -3.71+-0.26 | -0.62+-0.26 | 2.74 |
Si I | ... | -2.78+-0.36 | 0.31+-0.36 | 4.73 |
Ca I | ... | -2.46+-0.22 | 0.63+-0.22 | 3.88 |
Sc II | ... | -3.03+-0.14 | 0.06+-0.14 | 0.37 |
Ti I | ... | -2.46+-0.22 | 0.63+-0.22 | 2.49 |
Ti II | ... | -2.93+-0.14 | 0.16+-0.14 | 2.28 |
V II | ... | <-2.33 | <0.76 | <1.67 |
Cr I | ... | -3.36+-0.2 | -0.27+-0.2 | 2.28 |
Mn I | ... | -3.47+-0.2 | -0.38+-0.2 | 1.96 |
Mn II | ... | -3.60+-0.21 | -0.51+-0.21 | 2.08 |
Fe I | ... | -3.09+-0.22 | ... | 4.41 |
Fe II | ... | -2.84+-0.15 | ... | 4.66 |
Co I | ... | -3.08+-0.26 | 0.01+-0.26 | 1.91 |
Ni I | ... | -3.04+-0.23 | 0.05+-0.23 | 3.17 |
Zn I | ... | <-2.22 | <0.87 | <2.38 |
Sr II | ... | -3.40+-0.19 | -0.31+-0.19 | -0.28 |
Y II | ... | -3.39+-0.25 | -0.3+-0.25 | -0.93 |
Nb II | ... | <-0.02 | <3.07 | <1.4 |
Mo I | ... | <-0.82 | <2.27 | <1.1 |
Ba II | ... | -3.66+-0.14 | -0.57+-0.14 | -1.23 |
Ce II | ... | <-1.69 | <1.40 | <-0.11 |
Pr II | ... | <-1.09 | <2.00 | <-0.38 |
Nd II | ... | <-1.58 | <1.51 | <-0.08 |
Sm II | ... | <-1.10 | <1.99 | <-0.09 |
Eu II | ... | <-1.86 | <1.23 | <-1.35 |
Gd II | ... | <-0.86 | <2.23 | <0.26 |
Tb II | ... | <-0.23 | <2.86 | <-0.33 |
Dy II | ... | <-1.46 | <1.63 | <-0.32 |
Ho II | ... | <-0.85 | <2.24 | <-0.59 |
Er II | ... | <-1.10 | <1.99 | <-0.17 |
Tm II | ... | <-0.77 | <2.32 | <-0.77 |
Yb II | ... | <-2.14 | <0.95 | <-1.06 |
Hf II | ... | <-0.40 | <2.69 | <0.48 |
Pb I | ... | <-0.50 | <2.59 | <1.45 |
Th II | ... | <-0.37 | <2.72 | <-0.37 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)