CWWDL 2693
Summary
CWWDL 2693 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 very 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=0.92) 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) | 118.693 | -24.065 | 0.24 | -2.475 | 3.031 | – |
| UCC | 118.673 | -24.067 | 0.23 | -2.542 | 3.042 | 113.91 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=5.78, Z=0.44 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 2690 | 8.0 | 118.87 | -24.01 | 0.25 | -2.25 | 2.89 | 105.92 | 0.08 |
| UBC 462 | 8.0 | 118.88 | -24.06 | 0.29 | -2.65 | 3.06 | – | 0.19 |