CWNU 3297
Summary
CWNU 3297 is a poorly populated, very dense object of intermediate C3 quality. It is located at a large distance from the Sun, well 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) | 106.979 | -18.925 | 0.116 | -0.36 | 1.688 | – |
| UCC | 106.979 | -18.93 | 0.108 | -0.359 | 1.694 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.85, m-M=14.45, logA=8.9 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1835 | 77.8 | 106.98 | -18.93 | 0.1 | -0.35 | 1.7 | – | 0.53 |