HSC 1991
Summary
HSC 1991 is a poorly populated, very loose object of low 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) | 105.128 | -36.586 | 6.653 | -3.163 | -6.97 | 22.071 |
| Cavallo et al. (2024) | 106.05 | -38.948 | 6.697 | – | – | – |
| Hu & Soubiran (2025) | 106.05 | -38.948 | – | – | – | – |
| UCC | 106.599 | -39.228 | 6.583 | -3.471 | -6.797 | 28.258 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.054, diffAV50=0.369, MOD50=5.825, logAge50=8.127 |
| Cavallo et al. (2024) | AV50=0.3, dMod50=5.88, logAge50=9.15, [Fe/H]50=0.25 |
| Hu & Soubiran (2025) | MA23f=-0.17, MK24=-0.03, MF24=-0.45 |
Search coordinates in Bayestar19
