DBSB 120
Summary
DBSB 120 is a poorly populated, loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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) | 260.803 | -37.758 | – | 2.76 | -0.47 | – |
| UCC | 260.787 | -37.766 | 0.513 | -0.212 | -1.513 | -5.151 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.103, distance=5483, log_age=6.0 |
Search coordinates in Bayestar19