CWNU 3967
Summary
CWNU 3967 is a poorly populated, dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 270.724 | -22.815 | 0.274 | -0.964 | -2.376 | 843.71 |
| UCC | 270.737 | -22.815 | 0.262 | -0.967 | -2.379 | 41.247 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.95, m-M=12.9, logA=6.5 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 72 | 43.2 | 270.71 | -22.81 | 0.31 | -1.07 | -2.52 | 63.25 | 0.39 |