Table 1
Excerpt from the list of C, N, and O abundances for our sample of 181 stars.
| ID | Vbroad | [C/Fe] | [C/Fe] | [C/Fe] | [C/Fe] | [C/Fe] | [C/Fe] | [N/Fe] | [O/Fe] |
|---|---|---|---|---|---|---|---|---|---|
| [km s−1] | λ5128 | λ5165 | λ5380 | λ5052EW | λ5380EW | λ4215 | λ6300 | ||
| CoRoT-10 | 3.1 | 0.09 ± 0.03 | 0.01 ± 0.04 | … | … | … | 0.06 ± 0.02 | 0.09 ± 0.12 | … |
| CoRoT-2 | 9.8 | −0.05 ± 0.07 | −0.07 ± 0.09 | −0.13 ± 0.15 | −0.08 ± 0.12 | −0.10 ± 0.14 | −0.07 ± 0.05 | … | 0.11 ± 0.12 |
| … | … | … | … | … | … | … | … | … | … |
| XO-4 | 11.6 | 0.11 ± 0.12 | 0.11 ± 0.18 | 0.07 ± 0.13 | 0.03 ± 0.12 | 0.08 ± 0.14 | 0.08 ± 0.07 | … | … |
| XO-5 | 3.5 | 0.09 ± 0.05 | 0.08 ± 0.06 | 0.11 ± 0.12 | 0.10 ± 0.12 | 0.17 ± 0.14 | 0.09 ± 0.04 | 0.04 ± 0.12 | 0.07 ± 0.11 |
Notes. The first two columns give the target name and the average value of the composite of velocity fields (e.g. rotation and macroturbulent velocity) computed from single estimates. In the columns from 3 to 8, we list the carbon abundance ratios derived from each indicator plus the weighted mean and corresponding standard error, computed as explained in Sect. 3.1. The last two columns show the N and O abundance ratios. The complete table is available at the CDS.
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