HSC 1704
Summary
HSC 1704 is a poorly populated, dense object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 103.084 | -3.314 | 0.173 | -0.122 | 0.06 | 63.259 |
| Cavallo et al. (2024) | 103.104 | -3.322 | 0.171 | – | – | – |
| Hunt & Reffert (2024) | 103.084 | -3.314 | 0.173 | -0.122 | 0.06 | 63.259 |
| Hu & Soubiran (2025) | 103.104 | -3.322 | – | – | – | – |
| UCC | 103.101 | -3.311 | 0.181 | -0.084 | 0.043 | 53.239 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.909, diffAV50=1.173, MOD50=13.353, logAge50=8.89 |
| Cavallo et al. (2024) | AV50=2.02, dMod50=13.72, logAge50=9.14, [Fe/H]50=-0.46 |
| Hunt & Reffert (2024) | MassJ=532.411, MassTot=672.187 |
| Hu & Soubiran (2025) | MA22=-0.29, MA23f=-0.47, MA23g=-0.41, MK24=-0.3, MF24=-0.42 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3345 | 80.0 | 103.1 | -3.31 | 0.18 | -0.09 | 0.01 | 53.13 | 0.07 |
