CWNU 4412
Summary
CWNU 4412 is a poorly populated, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 94.58 | 4.622 | 0.26 | -0.488 | -0.433 | 60.73 |
| UCC | 94.581 | 4.619 | 0.278 | -0.483 | -0.436 | 60.729 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.25, m-M=13.15, logA=8.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1613 | 88.9 | 94.58 | 4.62 | 0.28 | -0.47 | -0.43 | 60.73 | 0.41 |