CWNU 4682
Summary
CWNU 4682 is a sparse, very loose object of intermediate 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) | 261.773 | -39.8 | 0.249 | -1.566 | -3.675 | – |
| UCC | 261.766 | -39.788 | 0.24 | -1.557 | -3.675 | -116.958 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.6, m-M=12.65, logA=9.6 |
Search coordinates in Bayestar19