CWNU 442
Summary
CWNU 442 is a moderately populated, moderately dense object of very high 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 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. (2022) | 63.087 | 31.286 | 2.78 | 3.59 | -5.72 | 32.2 |
| UCC | 63.188 | 31.597 | 2.781 | 3.68 | -5.653 | 19.868 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.35, m-M=7.4, logAge=7.3, Z=0.018 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 31 | 11.3 | 60.98 | 32.35 | 2.74 | 3.75 | -5.38 | 18.67 | 0.72 |
| OCSN 285 | 7.0 | 60.52 | 32.25 | 2.69 | 3.6 | -5.24 | 20.31 | 0.31 |