CWNU 345
Summary
CWNU 345 is a poorly populated, very loose object of low C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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 |
|---|---|---|---|---|---|---|
| He et al. (2022) | 18.928 | 71.177 | 1.02 | 2.33 | 0.33 | 20.7 |
| UCC | 18.894 | 71.182 | 1.0 | 2.298 | 0.343 | 9.558 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.95, m-M=10.4, logAge=7.9, Z=0.038 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 3502 | 80.0 | 18.9 | 71.23 | 1.0 | 2.31 | 0.36 | 20.14 | 0.01 |