HSC 1692
Summary
HSC 1692 is a poorly populated, very loose object of 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) | 83.218 | -11.289 | 3.792 | -1.194 | 6.963 | 9.026 |
| Cavallo et al. (2024) | 82.711 | -11.999 | 3.789 | – | – | – |
| UCC | 83.323 | -11.42 | 3.774 | -1.334 | 6.823 | 0.435 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.498, diffAV50=0.433, MOD50=7.087, logAge50=7.763 |
| Cavallo et al. (2024) | AV50=1.03, dMod50=7.04, logAge50=7.8, [Fe/H]50=0.03 |
Search coordinates in Bayestar19
