DBSB 66
Summary
DBSB 66 is a poorly populated, very loose object of very 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.
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) | 169.11 | -61.485 | – | -11.49 | 2.16 | – |
| UCC | 169.201 | -61.463 | 0.311 | -7.59 | 2.222 | -14.393 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.999, distance=7511, log_age=6.0 |
Search coordinates in Bayestar19