CWNU 3445
Summary
CWNU 3445 is a poorly populated, loose object of very low C3 quality. It is located at a large distance from the Sun, above 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) | 26.013 | 65.133 | 0.116 | -1.035 | 0.523 | -88.95 |
| UCC | 26.007 | 65.141 | 0.135 | -1.044 | 0.529 | -94.966 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.95, m-M=14.2, logA=8.9 |
Search coordinates in Bayestar19