CWNU 4666
Summary
CWNU 4666 is a sparse, 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: 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) | 178.395 | -63.148 | 0.139 | -6.055 | 1.056 | – |
| UCC | 178.397 | -63.137 | 0.141 | -6.069 | 1.059 | -14.03 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.95, m-M=15.6, logA=6.2 |
Search coordinates in Bayestar19