CWNU 2457
Summary
CWNU 2457 is a poorly populated, very loose object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.
This object shares a moderate percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 209.711 | -63.155 | 0.501 | -6.647 | -3.25 | – |
| UCC | 209.726 | -63.17 | 0.507 | -6.655 | -3.28 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.25, m-M=11.35, logAge=8.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 3319 | 42.9 | 209.18 | -63.29 | 0.5 | -6.69 | -3.21 | 0.39 | 0.15 |