CWNU 4129
Summary
CWNU 4129 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 348.305 | 60.923 | 0.314 | -3.533 | -2.073 | – |
| UCC | 348.231 | 60.894 | 0.317 | -3.565 | -2.079 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.2, m-M=12.25, logA=8.0 |
Search coordinates in Bayestar19