HSC 1724
Summary
HSC 1724 is a poorly populated, very 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) | 110.154 | -2.005 | 6.465 | -0.239 | -12.394 | 17.417 |
| Cavallo et al. (2024) | 109.929 | -1.937 | 6.518 | – | – | – |
| Hu & Soubiran (2025) | 109.929 | -1.937 | – | – | – | – |
| UCC | 110.273 | -1.387 | 6.299 | -0.338 | -12.449 | 23.045 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.107, diffAV50=0.54, MOD50=5.927, logAge50=9.168 |
| Cavallo et al. (2024) | AV50=0.47, dMod50=5.98, logAge50=8.85, [Fe/H]50=0.5 |
| Hu & Soubiran (2025) | MA22=-0.17, MA23f=-0.43, MK24=-0.02, MF24=-0.65 |
Search coordinates in Bayestar19
