CWNU 3429
Summary
CWNU 3429 is a poorly populated, very loose object of 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) | 158.769 | -55.188 | 0.138 | -6.23 | 3.03 | 30.22 |
| UCC | 158.765 | -55.185 | 0.168 | -6.25 | 3.026 | 30.22 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.9, m-M=14.05, logA=8.4 |
Search coordinates in Bayestar19