UBC 1392
Summary
UBC 1392 is a poorly populated, very loose object of high C3 quality. It is located at a large 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 |
|---|---|---|---|---|---|---|
| Castro-Ginard et al. (2022) | 118.03 | -25.53 | 0.16 | -2.17 | 3.12 | – |
| UCC | 118.048 | -25.495 | 0.159 | -2.153 | 3.147 | 89.36 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Castro-Ginard et al. (2022) | AV=0.6, Dist=5837, logAge=8.096 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 2822 | 92.6 | 118.04 | -25.49 | 0.16 | -2.15 | 3.15 | 89.36 | 0.08 |