CWNU 4555
Summary
CWNU 4555 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) | 333.443 | 57.77 | 0.13 | -2.578 | -1.901 | – |
| UCC | 333.435 | 57.77 | 0.124 | -2.57 | -1.901 | -87.201 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.55, m-M=16.1, logA=6.7 |
Search coordinates in Bayestar19