UFMG 67
Summary
UFMG 67 is a poorly populated, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is rarely studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Ferreira et al. (2021) | 262.32 | -30.95 | 0.955 | 3.806 | -0.296 | – |
| UCC | 262.264 | -30.89 | 0.95 | 3.8 | -0.287 | -16.653 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Ferreira et al. (2021) | E(B-V)=0.38, Dmod=10.15, logt=8.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 2122 | 100.0 | 262.27 | -30.9 | 0.95 | 3.8 | -0.29 | -16.65 | 0.07 |