HSC 1690
Summary
HSC 1690 is a moderately populated, very dense object of high C3 quality. It is located at a moderate 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) | 101.658 | -2.093 | 0.208 | -0.353 | -0.272 | 86.756 |
| Cavallo et al. (2024) | 101.658 | -2.097 | 0.21 | – | – | – |
| Hunt & Reffert (2024) | 101.658 | -2.093 | 0.208 | -0.353 | -0.272 | 86.756 |
| UCC | 101.661 | -2.097 | 0.215 | -0.346 | -0.269 | 83.286 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.696, diffAV50=1.775, MOD50=13.18, logAge50=8.653 |
| Cavallo et al. (2024) | AV50=2.87, dMod50=13.23, logAge50=8.65, [Fe/H]50=-0.17 |
| Hunt & Reffert (2024) | MassJ=672.488, MassTot=754.596 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3096 | 84.2 | 101.66 | -2.1 | 0.21 | -0.31 | -0.3 | 83.29 | 0.03 |
