HSC 1072
Summary
HSC 1072 is a sparse, loose object of low C3 quality. It is located at a relatively close distance from the Sun, below 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) | 28.353 | 55.585 | 0.549 | -0.968 | -0.796 | 182.183 |
| Cavallo et al. (2024) | 28.293 | 55.591 | 0.548 | – | – | – |
| Hunt & Reffert (2024) | 28.353 | 55.585 | 0.549 | -0.968 | -0.796 | 182.183 |
| UCC | 28.295 | 55.603 | 0.552 | -0.989 | -0.787 | 182.181 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.009, diffAV50=0.784, MOD50=11.223, logAge50=7.961 |
| Cavallo et al. (2024) | AV50=1.31, dMod50=11.46, logAge50=7.55, [Fe/H]50=0.13 |
| Hunt & Reffert (2024) | MassJ=113.480, MassTot=112.361 |
Search coordinates in Bayestar19