CWNU 3400
Summary
CWNU 3400 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
Warning: This is very 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) | 282.99 | -0.443 | 0.233 | -0.98 | -1.686 | 46.23 |
| UCC | 282.986 | -0.443 | 0.23 | -0.977 | -1.69 | 46.131 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.35, m-M=12.6, logA=8.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 320 | 95.8 | 282.98 | -0.44 | 0.23 | -0.97 | -1.69 | 46.13 | 0.55 |