CWNU 4142
Summary
CWNU 4142 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) | 259.108 | -38.293 | 0.313 | -0.149 | -2.192 | 56.61 |
| UCC | 259.176 | -38.32 | 0.328 | -0.163 | -2.212 | -1.052 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.6, m-M=12.55, logA=6.7 |
Search coordinates in Bayestar19