CWNU 4411
Summary
CWNU 4411 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near 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) | 277.065 | -11.464 | 0.318 | -0.458 | -2.21 | 29.54 |
| UCC | 277.072 | -11.441 | 0.324 | -0.458 | -2.208 | 19.649 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=5.65, m-M=13.0, logA=8.2 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 215 | 86.2 | 277.07 | -11.45 | 0.32 | -0.46 | -2.21 | 29.54 | 0.48 |