HSC 966
Summary
HSC 966 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) | 8.975 | 61.366 | 0.855 | -1.02 | -1.491 | -38.08 |
| Cavallo et al. (2024) | 9.448 | 61.291 | 0.852 | – | – | – |
| UCC | 9.624 | 61.296 | 0.847 | -1.046 | -1.544 | -22.092 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.661, diffAV50=1.939, MOD50=10.227, logAge50=8.266 |
| Cavallo et al. (2024) | AV50=1.83, dMod50=10.55, logAge50=8.05, [Fe/H]50=0.3 |
Search coordinates in Bayestar19