CWNU 3415
Summary
CWNU 3415 is a poorly populated, very loose object of very low C3 quality. It is located at a large 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) | 79.848 | 33.651 | 0.187 | 0.882 | -0.008 | -10.55 |
| UCC | 79.867 | 33.646 | 0.195 | 0.882 | -0.008 | -10.549 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.1, 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 1353 | 76.7 | 79.86 | 33.65 | 0.2 | 0.88 | -0.01 | -10.55 | 0.22 |