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Table 3

C, N, and O abundances.

Star [Fe/H] [C/Fe] [N/Fe] [O/Fe] C/O

V1261 Oria −0.66 ± 0.09 0.39 ± 0.14 1 0.73 ± 0.11 2 0.54 ± 0.08 3 0.38
IT Virb −0.45 ± 0.25 0.55 1.39 ± 0.30 (50) 0.40 (1) 0.75
0.62 1.11 ± 0.20 (94) 0.60 (1) 0.90
56 Peg −0.45 ± 0.12 0.01 ± 0.23 (13) −0.17 ± 0.07 (82) 0.12 ± − (1) 0.63
DR Dra −0.14 ± 0.10 −0.23 ± 0.07 (8) −0.21 ± 0.09 (82) 0.15 ± − (1) 0.39
ζ Cyg −0.03 ± 0.08 −0.22 ± 0.13 (15) 0.11 ± 0.05 (94) 0.16 ± 0.06 (2) 0.44
IP Eri 0.09 ± 0.08 −0.14 ± 0.16 (18) −0.23 ± 0.06 (96) 0.14 ± − (1) 0.54
V1379 Aql −0.23 ± 0.12 −0.24 ± 0.13 (8) 0.21 ± 0.05 (29)
HR 5692 −0.08 ± 0.09 −0.24 ± 0.10 (10) −0.16 ± 0.08 (90) 0.20 ± − (1) 0.43
ζ Cap −0.08 ± 0.13 0.11 ± 0.05 (16) 0.38 ± 0.07 (85) 0.12 ± 0.08 (2) 0.79
63 Eri −0.18 ± 0.08 −0.12 ± 0.18 (13) 0.25 ± 0.05 (50) 0.31 ± 0.04 (6) 0.20
14 Aur C −0.11 ± 0.08 0.22 ± 0.03 (3) 0.25 ± 0.13 (4) 0.16 ± − (1) 0.72

Notes. Only the statistical uncertainties are given here. The number of lines used are given in parentheses.

(a)

For this star, we used the Fe abundance from Kovacs (1983) scaled to the solar value of Holweger (1979). CNO abundances are taken from Smith & Lambert (1990) and are relative to α Tau.

(b)

Two equally likely abundance sets are listed for IT Vir (see text).

(1)

From CO lines at 1.6 and 2.2 μm;

(2)

from CN lines at 2.2 μm;

(3)

from OH lines at 1.6 and 2.2 μm.

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