CWNU 3414
Summary
CWNU 3414 is a poorly populated, moderately dense object of low 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) | 62.565 | 47.844 | 0.226 | -0.381 | -0.892 | -72.04 |
| UCC | 62.561 | 47.846 | 0.243 | -0.379 | -0.895 | -72.036 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.95, m-M=12.9, logA=8.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1217 | 82.4 | 62.56 | 47.85 | 0.24 | -0.38 | -0.87 | -72.04 | 0.43 |