CWNU 4717
Summary
CWNU 4717 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above 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) | 327.448 | 59.506 | 0.101 | -2.343 | -1.609 | – |
| UCC | 327.448 | 59.487 | 0.116 | -2.311 | -1.606 | -122.799 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.95, m-M=14.05, logA=8.9 |
Search coordinates in Bayestar19