CWNU 1187
Summary
CWNU 1187 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large 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) | 291.025 | 53.824 | 2.201 | 1.075 | -2.07 | – |
| UCC | 291.352 | 53.677 | 2.181 | 1.068 | -2.085 | -26.146 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.65, logAge=7.95 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 708 | 96.0 | 290.92 | 53.23 | 2.19 | 1.05 | -2.18 | -24.95 | 0.18 |