CWWDL 10539
Summary
CWWDL 10539 is a sparse, very loose object of intermediate 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, 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=0.84) 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) | 15.225 | 63.571 | 0.37 | -2.419 | -0.384 | – |
| UCC | 15.376 | 63.587 | 0.353 | -2.443 | -0.414 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=5.7, Z=0.23 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| COIN-Gaia 29 | 16.0 | 15.52 | 63.65 | 0.34 | -2.67 | -0.35 | -27.03 | 0.53 |
| CWWDL 2604 | 8.0 | 15.91 | 63.43 | 0.33 | -2.32 | -0.41 | -73.39 | 0.06 |
| Berkeley 62 | 4.0 | 15.32 | 63.93 | 0.36 | -2.17 | -0.4 | -20.65 | 0.9 |