CWNU 3319
Summary
CWNU 3319 is a poorly populated, loose object of low 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) | 89.73 | 15.78 | 0.139 | 0.576 | -0.785 | 29.66 |
| UCC | 89.724 | 15.772 | 0.166 | 0.59 | -0.774 | 29.656 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.4, m-M=13.2, logA=9.2 |
Search coordinates in Bayestar19