CWNU 4157
Summary
CWNU 4157 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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) | 176.871 | -61.087 | 0.13 | -5.867 | 1.17 | -5.87 |
| UCC | 176.881 | -61.084 | 0.133 | -5.863 | 1.17 | 15.422 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.3, m-M=15.65, logA=7.8 |
Search coordinates in Bayestar19