CWNU 3150
Summary
CWNU 3150 is a poorly populated, very dense object of intermediate 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) | 320.053 | 44.434 | 0.232 | -4.224 | -3.694 | -26.72 |
| UCC | 320.054 | 44.429 | 0.226 | -4.238 | -3.684 | -26.724 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.3, m-M=12.8, logA=9.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 694 | 96.0 | 320.05 | 44.43 | 0.23 | -4.24 | -3.68 | -26.72 | 0.49 |