CWNU 323
Summary
CWNU 323 is a poorly populated, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a significant 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) | 124.477 | -55.608 | 0.96 | -1.24 | 1.53 | -6.4 |
| UCC | 124.453 | -55.642 | 0.957 | -1.237 | 1.53 | -3.0 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.8, m-M=9.65, logAge=9.2, Z=0.008 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 7593 | 64.1 | 124.32 | -55.64 | 0.96 | -1.24 | 1.53 | -2.55 | 0.0 |