CWNU 1986
Summary
CWNU 1986 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 89.083 | 11.295 | 0.401 | 1.276 | -1.638 | 16.8 |
| UCC | 89.124 | 11.3 | 0.399 | 1.254 | -1.634 | 16.804 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.45, m-M=11.7, logAge=9.7 |
Search coordinates in Bayestar19