CWNU 3180
Summary
CWNU 3180 is a moderately populated, very loose object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 75.86 | 42.396 | 0.16 | 0.169 | -0.266 | -2.08 |
| UCC | 75.863 | 42.397 | 0.152 | 0.15 | -0.246 | -2.08 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.65, m-M=13.95, logA=8.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FSR 0734 | 39.7 | 75.86 | 42.4 | 0.16 | 0.18 | -0.25 | -2.08 | 0.4 |