CWNU 3327
Summary
CWNU 3327 is a poorly populated, very dense object of intermediate C3 quality. It is located at a large distance from the Sun, well above 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) | 123.964 | -24.09 | 0.202 | -1.173 | 1.525 | 46.08 |
| UCC | 123.965 | -24.098 | 0.191 | -1.173 | 1.525 | 46.513 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.45, m-M=13.45, logA=9.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1962 | 83.9 | 123.97 | -24.1 | 0.2 | -1.18 | 1.53 | 46.08 | 0.59 |