CWNU 4756
Summary
CWNU 4756 is a poorly populated, very loose object of very low C3 quality. It is located at a large 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) | 151.403 | -51.264 | 0.127 | -4.608 | 2.968 | 43.92 |
| UCC | 151.376 | -51.248 | 0.113 | -4.615 | 2.968 | 43.921 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.3, m-M=14.05, logA=9.5 |
Search coordinates in Bayestar19