CWNU 2009
Summary
CWNU 2009 is a poorly populated, 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: 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) | 112.377 | -21.163 | 0.277 | -1.547 | 3.658 | – |
| UCC | 112.377 | -21.162 | 0.275 | -1.546 | 3.658 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=12.5, logAge=8.2 |
Search coordinates in Bayestar19