CWNU 1118
Summary
CWNU 1118 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near 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) | 345.805 | 57.336 | 0.892 | -1.128 | -1.468 | – |
| UCC | 345.751 | 57.299 | 0.849 | -1.222 | -1.539 | -25.403 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=1.45, logAge=8.95 |
Search coordinates in Bayestar19