CWWDL 10399
Summary
CWWDL 10399 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 351.055 | 61.275 | 0.285 | -3.815 | -1.785 | -54.102 |
| UCC | 351.286 | 61.32 | 0.293 | -3.852 | -1.839 | -58.12 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=7.82, Z=0.44 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 399 | 16.0 | 351.34 | 61.33 | 0.37 | -4.01 | -2.15 | -57.18 | 0.2 |