CWNU 3542
Summary
CWNU 3542 is a poorly populated, very dense object of intermediate 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) | 300.866 | 30.423 | 0.245 | -2.88 | -5.418 | 5.51 |
| UCC | 300.841 | 30.424 | 0.233 | -2.864 | -5.393 | 5.689 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.3, m-M=12.5, logA=7.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 543 | 30.8 | 300.84 | 30.44 | 0.22 | -2.81 | -5.35 | 5.69 | 0.22 |