CWNU 4687
Summary
CWNU 4687 is a poorly populated, 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: 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) | 281.891 | -4.641 | 0.202 | -1.877 | -4.382 | 79.76 |
| UCC | 281.879 | -4.632 | 0.202 | -1.877 | -4.396 | 67.584 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=7.6, m-M=12.85, logA=6.7 |
Search coordinates in Bayestar19