HSC 1709
Summary
HSC 1709 is a poorly populated, loose object of very low C3 quality. It is located at a very close distance from the Sun, near 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) | 93.09 | -8.811 | 4.787 | -1.118 | -20.898 | 6.917 |
| Cavallo et al. (2024) | 92.79 | -8.804 | 4.783 | – | – | – |
| UCC | 92.739 | -8.343 | 4.774 | -0.987 | -20.947 | 25.553 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.397, diffAV50=0.604, MOD50=6.659, logAge50=8.437 |
| Cavallo et al. (2024) | AV50=0.7, dMod50=6.57, logAge50=8.5, [Fe/H]50=0.33 |
Search coordinates in Bayestar19
