CWWDL 3451
Summary
CWWDL 3451 is a sparse, very loose object of very low 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 |
|---|---|---|---|---|---|---|
| Chi et al. (2023) | 149.67 | -60.888 | 0.246 | -5.611 | 3.894 | 12.977 |
| UCC | 149.741 | -60.889 | 0.219 | -5.58 | 3.872 | -39.245 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Chi et al. (2023) | logAge=8.48, Z=-0.88 |
Search coordinates in Bayestar19