Table 9.
Distances and ages for the binary systems in the present sample compared to those of the parent clusters.
| Binary | Distance (pc) | Age (Myr) | Cluster | Distance (pc) | Ref. | Age (Myr) | Ref. |
|---|---|---|---|---|---|---|---|
| V1034 Sco | 1460 ± 50 | 5.0–7.7 | 5.3–7.0 | NGC 6321 | 1538 ± 20 | 1 | 6.3 | 2 |
| GL Car | 2278 ± 63 | 2.0 ± 0.5 | NGC 3572a | 2444 ± 33 | 3 | 1–4 | 4 |
| V573 Car | 2466 ± 78 | 1.5–3.1 | 2.2–2.7 | Trumpler 16 | 2360 ± 505 | 5 | 2 ± 1 | 6 |
| V346 Cen | 2290 ± 60 | 10.5–16.0 | 10.7-16.0 | Stock 14 | 2439 ± 326 | 7 | 10 ± 2 | 7 |
Notes. The distances to the binary systems are from the present work (Table 8). The ages were calculated by Tkachenko et al. (2020) except GL Car for which the age is adopted from Giménez & Clausen (1986). Tkachenko et al. (2020) estimated the age for two options: assuming the components are individual stars, and constraining the age to be the same for both components. Both measurements are given, separated by a vertical line.
Reference. (1) Banyard et al. (2022); (2) Kuhn et al. (2017); (3) Clariá (1976); (4) Garcia (1994); (5) Göppl & Preibisch (2022); (6) Hur et al. (2012); (7) Paunzen & Netopil (2006).
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.