CWNU 270
Summary
CWNU 270 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a very small percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 108.882 | -52.303 | 1.7 | -4.23 | 8.71 | 4.6 |
| UCC | 109.016 | -52.222 | 1.679 | -4.243 | 8.601 | 15.019 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.25, m-M=8.8, logAge=8.0, Z=0.02 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 649 | 4.0 | 112.56 | -51.37 | 1.53 | -4.39 | 8.45 | 12.83 | 0.07 |