CWNU 4688
Summary
CWNU 4688 is a sparse, very loose object of very low C3 quality. It is located at a moderate 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) | 245.53 | -51.122 | 0.492 | -0.972 | -2.19 | – |
| UCC | 245.472 | -51.133 | 0.493 | -0.943 | -2.179 | -20.369 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.7, m-M=11.7, logA=8.9 |
Search coordinates in Bayestar19