HSC 1714
Summary
HSC 1714 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) | 77.721 | -16.006 | 4.683 | -10.224 | -1.504 | 20.128 |
| Cavallo et al. (2024) | 79.784 | -13.955 | 4.681 | – | – | – |
| UCC | 79.576 | -13.764 | 4.645 | -10.215 | -1.857 | 21.352 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.048, diffAV50=0.332, MOD50=6.645, logAge50=8.215 |
| Cavallo et al. (2024) | AV50=0.33, dMod50=6.71, logAge50=8.18, [Fe/H]50=0.33 |
Search coordinates in Bayestar19
