CWNU 4358
Summary
CWNU 4358 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, above 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) | 232.351 | -51.128 | 0.199 | -4.824 | -3.506 | – |
| UCC | 232.299 | -51.123 | 0.174 | -4.836 | -3.492 | -68.059 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.95, m-M=13.4, logA=9.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4352 | 5.9 | 232.15 | -51.13 | 0.16 | -4.65 | -3.24 | -19.46 | 0.05 |