HSC 789
Summary
HSC 789 is a sparse, very loose object of intermediate C3 quality. It is located at a 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) | 329.122 | 58.91 | 1.099 | -1.933 | -3.768 | -19.074 |
| Cavallo et al. (2024) | 329.173 | 59.181 | 1.101 | – | – | – |
| UCC | 329.157 | 59.126 | 1.093 | -1.947 | -3.748 | -13.408 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.617, diffAV50=1.312, MOD50=9.676, logAge50=6.669 |
| Cavallo et al. (2024) | AV50=1.84, dMod50=9.75, logAge50=6.78, [Fe/H]50=0.02 |
Search coordinates in Bayestar19