HSC 1785
Summary
HSC 1785 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) | 106.154 | -13.71 | 0.312 | -0.608 | -1.245 | – |
| Cavallo et al. (2024) | 106.115 | -13.779 | 0.312 | – | – | – |
| Hu & Soubiran (2025) | 106.115 | -13.779 | – | – | – | – |
| UCC | 106.141 | -13.715 | 0.315 | -0.588 | -1.255 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.576, diffAV50=0.956, MOD50=12.689, logAge50=8.59 |
| Cavallo et al. (2024) | AV50=1.36, dMod50=12.15, logAge50=9.05, [Fe/H]50=-0.14 |
| Hu & Soubiran (2025) | MA22=-0.24, MA23f=-0.31, MK24=-0.27, MF24=-0.41 |
Search coordinates in Bayestar19