CWNU 1077
Summary
CWNU 1077 is a moderately populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a small percentage of members with a later reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 11.266 | 2.144 | 8.376 | 17.273 | -13.475 | – |
| UCC | 9.495 | 1.899 | 8.434 | 17.548 | -14.392 | 15.682 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.35, logAge=8.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 749 | 23.5 | 6.06 | 2.71 | 8.23 | 18.26 | -14.78 | 12.49 | 0.06 |