CWNU 54
Summary
CWNU 54 is a sparse, very loose object of very low C3 quality. It is located at a close 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. (2022) | 120.406 | -54.297 | 1.34 | -3.3 | 6.26 | 16.9 |
| UCC | 120.639 | -54.28 | 1.333 | -3.237 | 6.267 | 25.56 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.5, m-M=9.5, logAge=8.9, Z=0.02 |
Search coordinates in Bayestar19