CWNU 1255
Summary
CWNU 1255 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, below 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. (2022) | 300.228 | 9.312 | 2.195 | -1.545 | -12.456 | – |
| UCC | 300.277 | 9.467 | 2.221 | -1.593 | -12.416 | -8.29 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.4, logAge=7.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 247 | 65.4 | 300.33 | 10.5 | 2.18 | -1.62 | -12.24 | -9.02 | 0.09 |
| NGC 6858 | 30.8 | 300.72 | 11.16 | 2.15 | -1.67 | -11.95 | -8.92 | 0.46 |