CWNU 1022
Summary
CWNU 1022 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very close 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. (2022) | 80.349 | -11.303 | 2.967 | -0.145 | -2.377 | – |
| UCC | 80.417 | -11.15 | 3.003 | -0.023 | -1.405 | 10.816 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.45, logAge=7.9 |
Search coordinates in Bayestar19