CWNU 4009
Summary
CWNU 4009 is a poorly populated, very loose object of high C3 quality. It is located at a large 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) | 114.933 | -29.607 | 0.134 | -1.292 | 2.239 | 88.34 |
| UCC | 114.929 | -29.605 | 0.117 | -1.288 | 2.256 | 112.47 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.75, m-M=14.3, logA=7.5 |
Search coordinates in Bayestar19