HSC 2180
Summary
HSC 2180 is a poorly populated, loose object of intermediate C3 quality. It is located at a close distance from the Sun, above 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) | 142.424 | -43.903 | 1.556 | -8.174 | -0.373 | 15.264 |
| Cavallo et al. (2024) | 142.719 | -43.731 | 1.556 | – | – | – |
| UCC | 142.646 | -43.753 | 1.571 | -8.222 | -0.398 | 16.749 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.249, diffAV50=0.85, MOD50=8.936, logAge50=7.426 |
| Cavallo et al. (2024) | AV50=0.65, dMod50=9.52, logAge50=6.86, [Fe/H]50=0.14 |
Search coordinates in Bayestar19
