UBC 1032
Summary
UBC 1032 is a sparse, very dense 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) | 279.57 | -9.27 | 0.29 | -1.47 | -3.1 | – |
| Hunt & Reffert (2023) | 279.575 | -9.274 | 0.29 | -1.435 | -3.05 | – |
| Cavallo et al. (2024) | 279.573 | -9.27 | 0.287 | – | – | – |
| Hunt & Reffert (2024) | 279.575 | -9.274 | 0.29 | -1.435 | -3.05 | – |
| UCC | 279.573 | -9.279 | 0.293 | -1.456 | -3.086 | 19.605 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Castro-Ginard et al. (2022) | AV=3.007, Dist=3600, logAge=7.513 |
| Hunt & Reffert (2023) | AV50=3.89, diffAV50=2.242, MOD50=12.472, logAge50=7.452 |
| Cavallo et al. (2024) | AV50=3.72, dMod50=12.18, logAge50=7.66, [Fe/H]50=-0.27 |
| Hunt & Reffert (2024) | MassJ=522.135, MassTot=691.968 |
Search coordinates in Bayestar19
