HSC 1065
Summary
HSC 1065 is a poorly populated, very loose 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) | 29.599 | 59.635 | 0.235 | -1.294 | -0.256 | -82.424 |
| Cavallo et al. (2024) | 29.654 | 59.609 | 0.239 | – | – | – |
| Hunt & Reffert (2024) | 29.599 | 59.635 | 0.235 | -1.294 | -0.256 | -82.424 |
| Hu & Soubiran (2025) | 29.654 | 59.609 | – | – | – | – |
| UCC | 29.601 | 59.645 | 0.25 | -1.315 | -0.231 | -50.881 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.774, diffAV50=1.906, MOD50=12.735, logAge50=7.979 |
| Cavallo et al. (2024) | AV50=1.27, dMod50=12.72, logAge50=8.75, [Fe/H]50=0.67 |
| Hunt & Reffert (2024) | MassJ=329.186, MassTot=459.452 |
| Hu & Soubiran (2025) | MA22=-0.17, MA23f=-0.41, MK24=-0.23, MF24=-0.45 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3454 | 84.0 | 29.6 | 59.64 | 0.25 | -1.31 | -0.22 | -50.88 | 0.04 |
