CWNU 2351
Summary
CWNU 2351 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) | 123.992 | -43.34 | 0.29 | -3.217 | 4.24 | – |
| UCC | 123.93 | -43.341 | 0.27 | -3.27 | 4.235 | 87.469 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.95, m-M=13.2, logAge=6.3 |
Search coordinates in Bayestar19