CWNU 4811
Summary
CWNU 4811 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) | 84.594 | 20.187 | 0.107 | 0.53 | -0.679 | – |
| UCC | 84.622 | 20.171 | 0.112 | 0.464 | -0.658 | 7.517 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.25, m-M=14.75, logA=8.0 |
Search coordinates in Bayestar19