Table 3.
Carbon, nitrogen and oxygen abundances obtained from our analysis, and the best-fitting vmic for the CNO lines.
# | Name | Sp. class. | vmic | ϵC | # C | ϵN | # N | ϵO | # O |
---|---|---|---|---|---|---|---|---|---|
Dwarfs | |||||||||
1 | HD36512 | O9.7 V | ≤5 | ![]() |
7 | ![]() |
10 | ![]() |
10 |
2 | HD34078 | O9.5 V | 7.5 | ![]() |
6 | ![]() |
8 | ![]() |
7 |
3 | HD46202 | O9.2 V | 7.5 | ![]() |
7 | ![]() |
8 | ![]() |
8 |
4 | HD214680 | O9 V | 7.5 | ![]() |
8 | ![]() |
9 | ![]() |
9 |
5 | HD97848 | O8 V | 7.5 | ![]() |
5 | ![]() |
7 | ![]() |
8 |
6 | HD46966 | O8.5 IV | 7.5 | ![]() |
9 | ![]() |
7 | ![]() |
9 |
7 | HD93222 | O7 V((f)) | 10 | ![]() |
7 | ![]() |
8 | ![]() |
4 |
8 | HD12993 | O6.5 V((f)) Nstr | ≥20 | ![]() |
6 | ![]() |
7 | ![]() |
3 |
9 | HD303311 | O6 V((f))z | ≥20 | ![]() |
6 | ![]() |
5 | ![]() |
3 |
10 | HD96715 | O4 V((f))z | 20 | ![]() |
3 | ![]() |
8 | ![]() |
2 |
Supergiants and bright giants | |||||||||
12 | HD195592 | O9.7 Ia | 15 | ![]() |
6 | ![]() |
7 | ![]() |
5 |
13 | HD152249 | OC9 Iab | 15 | ![]() |
8 | ![]() |
8 | ![]() |
10 |
14 | HD71304 | O8.7 II | 15 | ![]() |
7 | ![]() |
7 | ![]() |
6 |
15 | HD207198 | O8.5 II(f) | 15 | ![]() |
5 | ![]() |
7 | ![]() |
7 |
16 | HD225160 | O8 Iabf | 10 | ![]() |
5 | ![]() |
6 | ![]() |
3 |
17 | HD171589 | O7.5 II(f) | 15 | ![]() |
7 | ![]() |
7 | ![]() |
3 |
18 | HD151515 | O7 II(f) | ≥20 | ![]() |
4 | ![]() |
8 | ![]() |
2 |
19 | HD169582 | O6 Iaf | ≥20 | ![]() |
5 | ![]() |
8 | ![]() |
1 |
Notes. For each abundance, the (asymmetric) errors refer to the 1-σ errors derived from the distribution (first number), and to the approximate total error budget estimated from additionally accounting for typical uncertainties in the stellar parameters (second number, separated by |). The table also provides the number of lines used for the χ2 analysis of a specific object/atomic species. For comparison, the maximum number of lines (for all ions) considered in our spectrum synthesis is 12 for carbon, 17 for nitrogen, and 10 for oxygen. The oxygen abundances for (at least) the cooler dwarfs (#1 to #5) should be considered with caution, since they might be affected by an imperfect model atom (see text).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.