HSC 1766
Summary
HSC 1766 is a poorly populated, loose object of intermediate C3 quality. It is located at a very 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) | 85.954 | -20.146 | 8.943 | 15.278 | -5.323 | 25.416 |
| Cavallo et al. (2024) | 84.904 | -19.387 | 8.908 | – | – | – |
| UCC | 85.837 | -19.507 | 8.844 | 15.031 | -5.371 | 26.12 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.558, diffAV50=0.658, MOD50=5.213, logAge50=7.503 |
| Cavallo et al. (2024) | AV50=0.96, dMod50=5.26, logAge50=8.11, [Fe/H]50=0.36 |
Search coordinates in Bayestar19
