CWNU 2722
Summary
CWNU 2722 is a poorly populated, very loose object of high C3 quality. It is located at a relatively 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. (2023) | 280.603 | -11.291 | 0.563 | 0.657 | -0.818 | – |
| UCC | 280.56 | -11.333 | 0.562 | 0.66 | -0.823 | 13.845 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.0, m-M=11.1, logAge=7.5 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 224 | 11.5 | 280.24 | -11.76 | 0.56 | 0.67 | -0.71 | – | 0.25 |