CWNU 539
(OCSN 161)
Summary
CWNU 539 is a poorly populated, loose object of low C3 quality. It is located at a very close distance from the Sun, below 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) | 103.814 | -37.54 | 2.22 | -8.94 | 10.48 | 27.1 |
| Qin et al. (2023) | 103.83 | -37.6 | 2.18 | -8.61 | 10.32 | 28.63 |
| UCC | 103.785 | -37.565 | 2.227 | -8.944 | 10.485 | 29.394 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.2, m-M=7.8, logAge=7.7, Z=0.006 |
| Qin et al. (2023) | E(B-V)=0.17, m-M=8.74, logt=8.4 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 249 | 80.0 | 103.76 | -37.56 | 2.23 | -8.87 | 10.52 | 28.76 | 0.02 |