CWNU 1091
Summary
CWNU 1091 is a poorly 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 significant 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) | 332.61 | 12.116 | 5.238 | 14.904 | -10.696 | – |
| UCC | 333.23 | 12.605 | 5.255 | 15.085 | -10.85 | -2.469 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.25, logAge=8.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 598 | 59.3 | 335.01 | 13.29 | 5.31 | 15.51 | -11.2 | 5.54 | 0.06 |