Table 5.
Comparison of abundances determined for targets in the present work to those of their parent clusters.
| NGC 6231 | |||
|---|---|---|---|
| Element | Kilian et al. (1994) | Mathys et al. (2002) | This work |
| V1034 Sco | |||
| log ϵ(C) | 8.37±0.05 | 8.29±0.17 | 8.33±0.08 |
| log ϵ(N) | 7.85±0.05 | 7.85±0.10 | 7.69±0.08 |
| log ϵ(O) | 8.61±0.05 | 8.30±0.42 | 8.73±0.12 |
| log ϵ(Mg) | 7.39±0.04 | – | 7.56±0.11 |
| log ϵ(Si) | 7.15±0.06 | – | 7.51±0.10 |
| [N/C] | −0.52±0.07 | −0.44±0.20 | −0.64±0.11 |
| [N/O] | −0.76±0.07 | −0.45±0.40 | −1.04±0.14 |
| NGC 3293 | |||
| Element | Hunter et al. (2009) | Morel et al. (2022) | V573 Car |
| GL Car | |||
| log ϵ(C) | 7.97±0.19 | 8.13±0.16 | 8.24±0.17 |
| log ϵ(N) | 7.60±0.15 | 7.72±0.14 | 7.70±0.27 |
| log ϵ(O) | 8.65±0.17 | – | 8.70±0.18 |
| log ϵ(Mg) | 7.22±0.16 | 7.45±0.18 | 7.50±0.20 |
| log ϵ(Si) | 7.42±0.09 | 7.56±0.25 | 7.51±0.26 |
| [N/C] | −0.37±0.21 | −0.40±0.21 | −0.54±0.27 |
| [N/O] | −1.05±0.26 | – | −1.00±0.11 |
Notes. V1034 Sco is member of the open cluster NGC 6231 for which abundance analyses were published by Kilian et al. (1994) and Mathys et al. (2002). For the open clusters NGC 3572 and Trumpler 16, parent clusters of GL Car and V573 Car, respectively, no abundance studies are available. We used abundance studies of the open cluster NGC 3293, since it is part of the large Car OB1 complex, as are NGC 3572 and Trumpler 16.
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.