UFMG 89
Summary
UFMG 89 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Ferreira et al. (2021) | 269.3 | -27.59 | 0.403 | 0.29 | -1.896 | – |
| Hunt & Reffert (2023) | 269.279 | -27.607 | 0.36 | 0.309 | -2.011 | 41.108 |
| Cavallo et al. (2024) | 269.273 | -27.608 | 0.36 | – | – | – |
| Hunt & Reffert (2024) | 269.279 | -27.607 | 0.36 | 0.309 | -2.011 | 41.108 |
| UCC | 269.29 | -27.605 | 0.371 | 0.298 | -1.982 | 8.885 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Ferreira et al. (2021) | E(B-V)=1.22, Dmod=10.7, logt=8.5 |
| Hunt & Reffert (2023) | AV50=4.096, diffAV50=2.407, MOD50=12.031, logAge50=7.135 |
| Cavallo et al. (2024) | AV50=4.21, dMod50=11.37, logAge50=7.33, [Fe/H]50=-0.3 |
| Hunt & Reffert (2024) | MassJ=1057.48, MassTot=1057.48 |
Search coordinates in Bayestar19
