CWNU 4117
Summary
CWNU 4117 is a sparse, very loose object of low C3 quality. It is located at a large 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. (2023) | 102.095 | 1.376 | 0.207 | -0.245 | 0.175 | – |
| UCC | 102.11 | 1.368 | 0.196 | -0.251 | 0.156 | 80.233 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.55, m-M=13.3, logA=7.5 |
Search coordinates in Bayestar19