CWNU 3593
Summary
CWNU 3593 is a moderately populated, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
This object shares a very small percentage of members with at least one entry reported in the same catalogue.
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 |
|---|---|---|---|---|---|---|
| He et al. (2023) | 167.948 | -67.89 | 0.095 | -5.2 | 1.978 | 21.58 |
| UCC | 167.909 | -67.891 | 0.082 | -5.167 | 1.974 | 6.513 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.6, m-M=14.05, logA=9.8 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4856 | 1.8 | 168.23 | -67.75 | 0.23 | -5.52 | 1.77 | -21.62 | 0.04 |