CWNU 4153
Summary
CWNU 4153 is a poorly populated, very loose object of very 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) | 333.202 | 61.056 | 0.149 | -2.404 | -1.873 | – |
| UCC | 333.198 | 61.055 | 0.155 | -2.409 | -1.879 | -78.263 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.25, m-M=16.5, logA=6.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4615 | 8.0 | 333.22 | 60.83 | 0.16 | -2.41 | -1.81 | -73.57 | 0.05 |