HSC 1715
Summary
HSC 1715 is a poorly populated, loose object of 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) | 96.546 | -7.547 | 8.525 | 4.583 | -13.791 | 24.334 |
| Cavallo et al. (2024) | 96.562 | -7.561 | 8.484 | – | – | – |
| UCC | 96.684 | -7.511 | 8.365 | 4.2 | -13.685 | 26.443 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.565, diffAV50=0.638, MOD50=5.278, logAge50=7.213 |
| Cavallo et al. (2024) | AV50=0.86, dMod50=5.27, logAge50=8.0, [Fe/H]50=0.32 |
Search coordinates in Bayestar19
