CWNU 1188
Summary
CWNU 1188 is a poorly populated, moderately dense 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 2 later reported entries.
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) | 269.772 | 2.899 | 2.383 | 0.058 | -8.326 | – |
| UCC | 269.906 | 2.931 | 2.362 | 0.138 | -8.258 | -14.985 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=1.05, logAge=7.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 305 | 77.8 | 269.76 | 2.93 | 2.38 | 0.05 | -8.21 | -13.41 | 0.03 |
| HSC 297 | 3.7 | 270.7 | 2.76 | 1.94 | 0.42 | -8.66 | -4.84 | 0.12 |