CWNU 4622
Summary
CWNU 4622 is a sparse, very loose object of very 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: contains less than 25 stars with P>0.5 estimated.
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) | 163.014 | -60.644 | 0.239 | -7.303 | 2.976 | – |
| UCC | 163.01 | -60.653 | 0.225 | -7.301 | 2.987 | -27.5 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.5, m-M=12.85, logA=8.6 |
Search coordinates in Bayestar19