CWNU 3313
Summary
CWNU 3313 is a moderately populated, dense object of low C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 151.387 | -61.042 | 0.059 | -3.633 | 2.319 | – |
| UCC | 151.39 | -61.043 | 0.064 | -3.633 | 2.342 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.8, m-M=15.1, logA=9.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 69 | 14.0 | 151.5 | -61.05 | 0.11 | -3.66 | 2.39 | – | 0.05 |