CWWDL 4726
Summary
CWWDL 4726 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, below 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, and a very small percentage with at least one entry reported in the same catalogue.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.88) 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) | 111.572 | -20.654 | 0.337 | -2.274 | 2.913 | – |
| UCC | 111.566 | -20.714 | 0.328 | -2.248 | 2.96 | 154.807 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=7.07, Z=0.02 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 224 | 12.0 | 111.38 | -20.96 | 0.33 | -2.3 | 3.12 | 26.35 | 0.14 |
| CWWDL 635 | 4.0 | 111.42 | -20.74 | 0.32 | -2.17 | 3.09 | 154.81 | 0.07 |