CWNU 1992
Summary
CWNU 1992 is a poorly populated, loose object of intermediate C3 quality. It is located at a moderate 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) | 299.811 | 23.155 | 0.382 | -2.094 | -6.846 | – |
| UCC | 299.806 | 23.155 | 0.374 | -2.087 | -6.837 | 24.259 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.55, m-M=11.9, logAge=7.75 |
Search coordinates in Bayestar19