UBC 1091
Summary
UBC 1091 is a sparse, very loose object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a significant percentage of members with 2 later reported entries.
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 |
|---|---|---|---|---|---|---|
| Castro-Ginard et al. (2022) | 301.56 | 36.32 | 0.34 | -2.53 | -5.12 | – |
| UCC | 301.607 | 36.374 | 0.339 | -2.527 | -5.112 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Castro-Ginard et al. (2022) | AV=1.585, Dist=2994, logAge=7.543 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0103 | 72.0 | 301.61 | 36.42 | 0.35 | -2.54 | -5.11 | – | 0.18 |
| Theia 4725 | 68.0 | 301.61 | 36.42 | 0.34 | -2.54 | -5.1 | – | 0.07 |