CWNU 3444
Summary
CWNU 3444 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 113.596 | -13.62 | 0.2 | -1.374 | 1.836 | 90.31 |
| UCC | 113.594 | -13.649 | 0.2 | -1.372 | 1.868 | 77.28 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.75, m-M=13.2, logA=8.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1814 | 68.0 | 113.52 | -13.61 | 0.2 | -1.37 | 1.87 | 90.31 | 0.12 |
| ASCC 40 | 36.0 | 113.43 | -13.77 | 0.18 | -1.38 | 1.74 | 95.1 | 0.32 |