CWWDL 4607
Summary
CWWDL 4607 is a sparse, very loose object of high 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 a unique object, which shares a very small percentage of members with at least one previously reported entry, and a significant 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=0.96) 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) | 33.986 | 57.725 | 0.41 | -0.832 | -1.067 | – |
| UCC | 33.957 | 57.708 | 0.414 | -0.822 | -1.042 | 317.007 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=6.45, Z=0.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 13364 | 56.0 | 34.05 | 57.8 | 0.43 | -0.84 | -1.05 | 317.01 | 0.14 |
| UBC 46 | 4.0 | 33.69 | 57.31 | 0.4 | -0.83 | -1.16 | 13.37 | 0.27 |