HSC 1189
Summary
HSC 1189 is a sparse, very loose object of low 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.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 54.883 | 48.82 | 0.352 | 0.626 | -1.588 | -7.558 |
| Cavallo et al. (2024) | 54.833 | 48.966 | 0.354 | – | – | – |
| Hunt & Reffert (2024) | 54.883 | 48.82 | 0.352 | 0.626 | -1.588 | -7.558 |
| UCC | 54.798 | 48.867 | 0.343 | 0.598 | -1.578 | 0.029 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.219, diffAV50=0.821, MOD50=12.023, logAge50=8.372 |
| Cavallo et al. (2024) | AV50=1.28, dMod50=11.86, logAge50=8.35, [Fe/H]50=0.47 |
| Hunt & Reffert (2024) | MassJ=64.8242, MassTot=237.638 |
Search coordinates in Bayestar19
