CWNU 2092
Summary
CWNU 2092 is a sparse, very loose object of very 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) | 55.35 | 51.284 | 0.456 | 0.782 | -1.24 | -42.1 |
| UCC | 55.253 | 51.287 | 0.441 | 0.768 | -1.254 | -42.099 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.45, m-M=11.4, logAge=9.05 |
Search coordinates in Bayestar19