HSC 770
Summary
HSC 770 is a sparse, very 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) | 325.257 | 56.054 | 0.254 | -4.173 | -4.015 | – |
| Cavallo et al. (2024) | 325.316 | 55.969 | 0.252 | – | – | – |
| Hunt & Reffert (2024) | 325.257 | 56.054 | 0.254 | -4.173 | -4.015 | – |
| UCC | 325.337 | 55.944 | 0.259 | -4.206 | -4.02 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.193, diffAV50=0.904, MOD50=12.832, logAge50=7.264 |
| Cavallo et al. (2024) | AV50=2.88, dMod50=12.21, logAge50=7.58, [Fe/H]50=0.31 |
| Hunt & Reffert (2024) | MassJ=219.463, MassTot=181.129 |
Search coordinates in Bayestar19