CWNU 4465
Summary
CWNU 4465 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very 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) | 267.543 | -36.894 | 0.042 | -2.922 | -6.587 | -100.9 |
| UCC | 267.535 | -36.894 | 0.064 | -2.908 | -6.609 | -75.478 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.4, m-M=17.4, logA=8.9 |
Search coordinates in Bayestar19