HSC 1092
Summary
HSC 1092 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, above 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) | 40.657 | 65.44 | 0.328 | -1.057 | 0.253 | -35.782 |
| Cavallo et al. (2024) | 40.589 | 65.464 | 0.331 | – | – | – |
| Hunt & Reffert (2024) | 40.657 | 65.44 | 0.328 | -1.057 | 0.253 | -35.782 |
| UCC | 40.59 | 65.453 | 0.331 | -1.038 | 0.243 | -35.77 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.255, diffAV50=1.909, MOD50=12.119, logAge50=8.409 |
| Cavallo et al. (2024) | AV50=3.46, dMod50=12.32, logAge50=8.46, [Fe/H]50=0.01 |
| Hunt & Reffert (2024) | MassJ=212.672, MassTot=233.510 |
Search coordinates in Bayestar19
