UBC 672
Summary
UBC 672 is a sparse, very loose 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.
Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Cantat-Gaudin et al. (2020) | 253.128 | -41.525 | 0.565 | -0.645 | -2.009 | – |
| Celli et al. (2024) | 253.128 | -41.525 | – | – | – | – |
| UCC | 253.281 | -41.606 | 0.571 | -0.642 | -2.025 | -26.656 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Cantat-Gaudin et al. (2020) | AVNN=1.14, DistPc=1595.0, AgeNN=7.02 |
| Celli et al. (2024) | Age=10.5, Mc=287.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| NGC 6231 | 52.0 | 253.56 | -41.83 | 0.6 | -0.58 | -2.18 | -27.67 | 1.0 |
| CWWDL 14193 | 4.0 | 253.36 | -41.47 | 0.63 | -0.66 | -1.94 | -15.26 | 0.16 |