CWNU 4380
Summary
CWNU 4380 is a poorly populated, very loose object of low C3 quality. It is located at a very large distance from the Sun, well below 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) | 165.077 | -64.888 | 0.088 | -4.435 | 1.888 | 35.43 |
| UCC | 165.123 | -64.87 | 0.075 | -4.483 | 1.84 | 42.185 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.6, m-M=14.6, logA=9.5 |
Search coordinates in Bayestar19