CWNU 1196
(OCSN 123)
Summary
CWNU 1196 is a poorly populated, loose object of low C3 quality. It is located at a very close distance from the Sun, near 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) | 168.537 | -70.659 | 3.449 | -21.725 | -0.648 | – |
| Qin et al. (2023) | 169.02 | -70.85 | 3.52 | -21.99 | -1.01 | 3.7 |
| UCC | 168.386 | -70.638 | 3.45 | -21.725 | -0.648 | 4.719 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.6, logAge=7.6 |
| Qin et al. (2023) | E(B-V)=0.28, m-M=7.98, logt=7.75 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 2442 | 100.0 | 170.96 | -71.15 | 3.49 | -21.89 | -1.34 | 4.72 | 0.19 |