CWNU 4092
Summary
CWNU 4092 is a poorly populated, moderately dense 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) | 318.352 | 49.879 | 0.198 | -2.703 | -3.088 | – |
| UCC | 318.349 | 49.879 | 0.2 | -2.71 | -3.087 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.95, m-M=12.65, logA=7.3 |
Search coordinates in Bayestar19