CWNU 3418
Summary
CWNU 3418 is a poorly populated, very loose object of high 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) | 119.218 | -27.286 | 0.165 | -1.855 | 2.224 | 84.67 |
| UCC | 119.215 | -27.28 | 0.147 | -1.864 | 2.235 | 84.671 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.2, m-M=14.1, logA=7.8 |
Search coordinates in Bayestar19