CWNU 2455
Summary
CWNU 2455 is a poorly populated, very loose object of high C3 quality. It is located at a large distance from the Sun, near 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) | 115.944 | -23.672 | 0.186 | -1.331 | 2.062 | – |
| UCC | 115.938 | -23.659 | 0.181 | -1.34 | 2.038 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.7, m-M=13.55, logAge=7.8 |
Search coordinates in Bayestar19