CWNU 4185
Summary
CWNU 4185 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) | 165.784 | -56.085 | 0.17 | -6.038 | 2.434 | 4.41 |
| UCC | 165.801 | -56.095 | 0.14 | -6.033 | 2.399 | 16.886 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.05, m-M=13.7, logA=9.7 |
Search coordinates in Bayestar19