HSC 1856
Summary
HSC 1856 is a poorly populated, loose object of intermediate C3 quality. It is located at a close distance from the Sun, near the mid-plane. It was recently reported in the literature.
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) | 110.53 | -20.264 | 1.786 | -5.496 | 4.343 | 34.975 |
| Cavallo et al. (2024) | 110.403 | -20.306 | 1.789 | – | – | – |
| UCC | 110.561 | -20.252 | 1.787 | -5.569 | 4.359 | 32.922 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.304, diffAV50=0.716, MOD50=8.66, logAge50=7.936 |
| Cavallo et al. (2024) | AV50=0.0, dMod50=8.85, logAge50=8.1, [Fe/H]50=0.69 |
Search coordinates in Bayestar19
