CWNU 4275
Summary
CWNU 4275 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) | 355.295 | 59.614 | 0.188 | -2.181 | -1.158 | – |
| UCC | 355.303 | 59.617 | 0.194 | -2.134 | -1.168 | -97.677 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.15, m-M=13.0, logA=8.6 |
Search coordinates in Bayestar19