HSC 606
Summary
HSC 606 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, 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) | 320.837 | 28.136 | 2.576 | 6.735 | -6.381 | -6.0 |
| Cavallo et al. (2024) | 321.707 | 27.622 | 2.568 | – | – | – |
| UCC | 321.712 | 27.359 | 2.591 | 6.721 | -6.297 | -4.31 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.281, diffAV50=0.547, MOD50=7.876, logAge50=8.009 |
| Cavallo et al. (2024) | AV50=0.69, dMod50=7.93, logAge50=7.95, [Fe/H]50=0.02 |
Search coordinates in Bayestar19
