HSC 1710
Summary
HSC 1710 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) | 61.141 | -21.449 | 7.264 | 14.348 | 11.841 | 23.013 |
| Cavallo et al. (2024) | 62.566 | -23.457 | 7.182 | – | – | – |
| UCC | 62.647 | -23.513 | 7.153 | 15.631 | 11.338 | 26.942 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.074, diffAV50=0.335, MOD50=5.638, logAge50=8.097 |
| Cavallo et al. (2024) | AV50=0.62, dMod50=5.76, logAge50=7.89, [Fe/H]50=0.28 |
Search coordinates in Bayestar19
