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Table 3

Determined abundances and isotopic ratios for programme stars.

Star [C/Fe] σ [C/Fe] [N/Fe] σ [N/Fe] [O/Fe] σ [O/Fe] C/N 12C/13C Evol.

Collinder 261
RGB02 −0.20 0.04 0.16 0.02 −0.10 0.05 1.74 18 g
RGB05 −0.27 0.04 −0.01 0.05 −0.09 0.05 2.19 8 c
RGB06 −0.21 0.05 0.29 0.04 0.09 0.05 1.26 13 c
RGB07 −0.23 0.01 0.20 0.02 0.01 0.05 1.48 c
RGB09 −0.21 0.07 0.25 0.02 −0.04 0.05 1.38 12 c
RGB10 −0.20 0.03 0.17 0.01 −0.05 0.05 1.70 c
RGB11 −0.23 0.01 0.17 0.03 −0.11 0.05 1.58 12 c

Average: −0.23 ± 0.02 0.18 ± 0.09 −0.03 ± 0.07 1.60 ± 0.30 11 ± 2

Melotte 66
1346 −0.32 0.02 0.13 0.03 0.13 0.05 1.41 8 c
1493 −0.19 0.01 0.12 0.04 0.20 0.05 1.95 8 c
1785 −0.23 0.01 0.10 0.05 0.10 0.05 1.86 6 c
1884 −0.10 0.01 0.28 0.03 0.22 0.05 1.66 c
2218 −0.21 0.01 0.23 0.07 0.14 0.05 1.45 10 c

Average: −0.21 ± 0.07 0.17 ± 0.07 0.16 ± 0.04 1.67 ± 0.21 8 ± 2

Notes. Evol.: g – first ascent giant; c – He-core burning star. The first ascent giant RGB02 in Collinder 261 was not used for the average abundance calculations.

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