HSC 767
Summary
HSC 767 is a sparse, very loose object of low C3 quality. It is located at a relatively close 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) | 322.685 | 57.396 | 0.956 | -3.315 | -3.37 | -25.214 |
| Cavallo et al. (2024) | 322.496 | 57.249 | 0.956 | – | – | – |
| Hunt & Reffert (2024) | 322.685 | 57.396 | 0.956 | -3.315 | -3.37 | -25.214 |
| UCC | 322.535 | 57.301 | 0.954 | -3.3 | -3.35 | -25.197 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.41, diffAV50=2.013, MOD50=10.062, logAge50=7.753 |
| Cavallo et al. (2024) | AV50=2.74, dMod50=10.13, logAge50=7.86, [Fe/H]50=-0.47 |
| Hunt & Reffert (2024) | MassJ=82.3026, MassTot=114.340 |
Search coordinates in Bayestar19