CWNU 3413
Summary
CWNU 3413 is a poorly populated, loose object of high 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 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) | 14.684 | 60.724 | 0.352 | -2.526 | -0.786 | – |
| UCC | 14.657 | 60.73 | 0.352 | -2.526 | -0.79 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.35, m-M=12.05, logA=7.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 2924 | 100.0 | 14.63 | 60.73 | 0.35 | -2.52 | -0.79 | – | 0.37 |