BDSB 125
Summary
BDSB 125 is a moderately populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.89) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 281.517 | -2.655 | – | 1.29 | -8.99 | – |
| UCC | 281.465 | -2.729 | 0.244 | -1.172 | -3.72 | 28.108 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=2.082, distance=6699, log_age=6.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| MCM 11 | 10.7 | 281.66 | -2.77 | 0.18 | -1.14 | -3.82 | – | 0.03 |
| CWNU 3930 | 1.8 | 281.31 | -2.8 | 0.21 | -1.52 | -3.85 | 47.3 | 0.17 |
| Ryu 912 | 1.8 | 281.32 | -2.8 | 0.19 | -1.54 | -3.86 | – | 0.39 |