CWNU 4167
Summary
CWNU 4167 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, below 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) | 311.304 | 36.203 | 0.121 | -2.47 | -3.678 | -86.7 |
| UCC | 311.287 | 36.187 | 0.13 | -2.498 | -3.674 | -79.726 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.85, m-M=14.45, logA=9.2 |
Search coordinates in Bayestar19