CWNU 1958
Summary
CWNU 1958 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 244.232 | -51.963 | 0.319 | -3.7 | -4.347 | – |
| UCC | 244.27 | -51.952 | 0.315 | -3.692 | -4.356 | -41.519 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.8, m-M=13.0, logAge=6.65 |
Search coordinates in Bayestar19