CWNU 291
Summary
CWNU 291 is a poorly populated, very loose object of high C3 quality. It is located at a close distance from the Sun, above 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) | 255.398 | -25.677 | 1.02 | -0.55 | 0.34 | – |
| UCC | 255.37 | -25.716 | 1.022 | -0.539 | 0.342 | -15.249 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.55, m-M=9.95, logAge=7.9, Z=0.02 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 3329 | 68.0 | 255.37 | -25.69 | 1.02 | -0.6 | 0.3 | -18.55 | 0.15 |