CWNU 4133
Summary
CWNU 4133 is a poorly populated, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
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) | 278.527 | -19.613 | 0.124 | -3.226 | -5.33 | 8.36 |
| UCC | 278.551 | -19.612 | 0.132 | -3.224 | -5.332 | -9.591 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.35, m-M=15.7, logA=9.6 |
Search coordinates in Bayestar19