CWNU 4493
Summary
CWNU 4493 is a poorly populated, loose object of low C3 quality. It is located at a moderate 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) | 343.017 | 57.151 | 0.282 | -3.169 | -2.629 | – |
| UCC | 342.993 | 57.149 | 0.274 | -3.171 | -2.608 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.05, m-M=12.55, logA=6.3 |
Search coordinates in Bayestar19