CWNU 4322
Summary
CWNU 4322 is a poorly populated, very loose object of high C3 quality. It is located at a large 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) | 247.932 | -52.568 | 0.122 | -4.578 | -4.865 | -122.21 |
| UCC | 247.912 | -52.572 | 0.111 | -4.56 | -4.891 | -75.937 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.35, m-M=15.55, logA=9.2 |
Search coordinates in Bayestar19