CWNU 4265
Summary
CWNU 4265 is a moderately populated, very loose object of very low C3 quality. It is located at a large distance from the Sun, below 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) | 102.69 | -3.591 | 0.168 | -0.54 | 0.922 | – |
| UCC | 102.69 | -3.589 | 0.165 | -0.535 | 0.922 | 90.75 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.45, m-M=13.25, logA=7.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1706 | 45.8 | 102.69 | -3.61 | 0.17 | -0.51 | 0.9 | 105.34 | 0.28 |