HSC 2077
Summary
HSC 2077 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
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) | 122.455 | -42.173 | 0.064 | -1.295 | 2.106 | 96.208 |
| Cavallo et al. (2024) | 122.416 | -42.149 | 0.066 | – | – | – |
| UCC | 122.46 | -42.191 | 0.078 | -1.291 | 2.131 | 110.373 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.0, diffAV50=1.805, MOD50=15.137, logAge50=6.935 |
| Cavallo et al. (2024) | AV50=0.8, dMod50=14.67, logAge50=8.04, [Fe/H]50=0.3 |
Search coordinates in Bayestar19
