Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-0.46 | <5.05 | <0.70 |
Be II | ... | <-2.35 | <3.36 | <-1.20 |
CH | ... | -1.65 | 4.06 | 6.90 |
NH | ... | -1.18 | 4.53 | 6.79 |
OH | ... | -2.03 | 3.68 | 6.84 |
Na I | ... | -3.34 | 2.17 | 2.99 |
Mg I | ... | -4.04 | 1.67 | 3.54 |
Al I | ... | -4.57 | 0.94 | 1.90 |
Ca I | ... | -5.48 | 0.03 | 0.88 |
Ca II | ... | -5.02 | 0.69 | 1.34 |
Sc II | ... | <-4.85 | <0.86 | <-1.68 |
Ti II | ... | -5.11 | 0.40 | -0.09 |
V I | ... | <-2.50 | <3.21 | <1.50 |
Cr I | ... | <-5.22 | ... | <0.45 |
Mn I | ... | <-4.55 | <0.96 | <0.84 |
Fe I | ... | -5.71 | ... | 1.79 |
Fe II | ... | <-5.51 | ... | <1.99 |
Co I | ... | <-4.34 | <1.37 | <0.58 |
Ni I | ... | -5.52 | -0.01 | 0.73 |
Zn I | ... | <-2.99 | <2.52 | <1.61 |
Sr II | ... | -4.73 | 0.98 | -1.76 |
Ba II | ... | <-4.27 | <1.24 | <-2.14 |
Eu II | ... | <-1.27 | <4.44 | <-0.76 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)