CWNU 4675
Summary
CWNU 4675 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
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. (2023) | 101.258 | 5.207 | 0.216 | 0.056 | -0.354 | 84.47 |
| UCC | 101.269 | 5.253 | 0.201 | 0.067 | -0.303 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.65, m-M=13.2, logA=8.9 |
Search coordinates in Bayestar19