CWNU 1731
Summary
CWNU 1731 is a sparse, loose object of 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) | 47.682 | 53.808 | 0.398 | 0.61 | -1.296 | – |
| UCC | 47.647 | 53.822 | 0.347 | 0.567 | -1.33 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.65, m-M=12.45, logAge=6.2 |
Search coordinates in Bayestar19