CWNU 4677
Summary
CWNU 4677 is a sparse, very loose object of 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 |
|---|---|---|---|---|---|---|
| He et al. (2023) | 264.922 | -35.131 | 0.201 | -1.645 | -3.252 | -49.93 |
| UCC | 264.917 | -35.135 | 0.21 | -1.648 | -3.248 | -49.934 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.55, m-M=13.25, logA=9.1 |
Search coordinates in Bayestar19