Table 7: C, N, O and heavy elements. Carbon abundances are derived from C2 lines and nitrogen abundances from CN lines (Sect. 6). Abundances of the heavy elements Ba, La and Eu are derived using hyperfine structure (Sect. 4).
Species $\lambda ({\rm\AA})$ $\chi _{\rm ex}$(eV) log gf I-18 I-36 I-42
[OI] 6300.311 0.00 -9.716 +0.10 +0.15 +0.20
ScII 6300.67 1.50 hfs -0.25 -0.20 +0.00
C(C2) 5634.2, 35.5 (0, 1) - 0.00 0.00 0.00
N(CN) 6332.2 (5, 1) - +0.60 +0.60 +0.60
BaII 6141.727 0.70 -0.08 -0.05 +0.20 -0.05
BaII 6496.908 0.60 -0.38 0.00 +0.10 0.00
LaII 6390.480 0.32 -1.45 -0.30 -0.15 +0.00
EuII 6645.127 1.38 +0.12 +0.15 +0.15 +0.15


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