CWNU 3482
Summary
CWNU 3482 is a poorly populated, very loose object of high 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) | 100.053 | -5.838 | 0.119 | -0.259 | 0.855 | 80.22 |
| UCC | 100.058 | -5.826 | 0.119 | -0.289 | 0.893 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.2, m-M=13.75, logA=8.9 |
Search coordinates in Bayestar19