DBSB 60
Summary
DBSB 60 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is poorly studied in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 166.404 | -62.485 | – | -10.49 | 4.76 | – |
| Cantat-Gaudin et al. (2018) | 166.385 | -62.482 | 0.202 | -5.229 | 1.874 | – |
| Cantat-Gaudin et al. (2020) | 166.385 | -62.482 | 0.202 | -5.229 | 1.874 | – |
| Celli et al. (2024) | 166.385 | -62.482 | – | – | – | – |
| UCC | 166.355 | -62.476 | 0.178 | -5.269 | 1.854 | 34.157 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.353, distance=3740, log_age=6.75 |
| Cantat-Gaudin et al. (2018) | dmode=4321.3 |
| Celli et al. (2024) | Age=5.6, Mc=252.5 |
Search coordinates in Bayestar19