UBC 1490
Summary
UBC 1490 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Castro-Ginard et al. (2022) | 163.7 | -60.63 | 0.2 | -7.39 | 2.98 | -3.96 |
| Hunt & Reffert (2023) | 163.661 | -60.649 | 0.209 | -7.393 | 2.964 | -4.992 |
| Cavallo et al. (2024) | 163.673 | -60.632 | 0.208 | – | – | – |
| Hunt & Reffert (2024) | 163.661 | -60.649 | 0.209 | -7.393 | 2.964 | -4.992 |
| UCC | 163.689 | -60.64 | 0.207 | -7.38 | 2.984 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Castro-Ginard et al. (2022) | AV=1.304, Dist=5195, logAge=7.519 |
| Hunt & Reffert (2023) | AV50=1.34, diffAV50=2.107, MOD50=13.506, logAge50=8.256 |
| Cavallo et al. (2024) | AV50=1.19, dMod50=14.18, logAge50=8.38, [Fe/H]50=-0.43 |
| Hunt & Reffert (2024) | MassJ=311.681, MassTot=812.848 |
Search coordinates in Bayestar19
