CWWDL 12507
Summary
CWWDL 12507 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.84) 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 |
|---|---|---|---|---|---|---|
| Chi et al. (2023) | 78.115 | 45.395 | 0.286 | 0.76 | -1.523 | -41.04 |
| UCC | 78.105 | 45.33 | 0.286 | 0.667 | -1.482 | -7.563 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=7.85, Z=-0.28 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 2505 | 16.0 | 78.06 | 45.31 | 0.29 | 0.49 | -1.33 | -40.34 | 0.13 |