CWNU 4458
Summary
CWNU 4458 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) | 287.027 | 11.027 | 0.111 | -2.735 | -5.753 | 25.94 |
| UCC | 287.016 | 11.015 | 0.103 | -2.707 | -5.756 | 32.652 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.9, m-M=16.4, logA=8.9 |
Search coordinates in Bayestar19