CWNU 4210
Summary
CWNU 4210 is a sparse, moderately dense 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) | 98.303 | 2.691 | 0.202 | 0.263 | 0.318 | – |
| UCC | 98.311 | 2.694 | 0.226 | 0.268 | 0.321 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.0, m-M=14.55, logA=7.3 |
Search coordinates in Bayestar19