HSC 1835
Summary
HSC 1835 is a poorly populated, very dense object of intermediate C3 quality. It is located at a large distance from the Sun, well 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) | 106.982 | -18.928 | 0.107 | -0.345 | 1.692 | – |
| Cavallo et al. (2024) | 106.983 | -18.927 | 0.117 | – | – | – |
| Hunt & Reffert (2024) | 106.982 | -18.928 | 0.107 | -0.345 | 1.692 | – |
| Hu & Soubiran (2025) | 106.983 | -18.927 | – | – | – | – |
| UCC | 106.979 | -18.929 | 0.101 | -0.35 | 1.695 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.723, diffAV50=1.776, MOD50=14.281, logAge50=9.015 |
| Cavallo et al. (2024) | AV50=1.89, dMod50=14.21, logAge50=8.94, [Fe/H]50=-0.08 |
| Hunt & Reffert (2024) | MassJ=902.931, MassTot=902.931 |
| Hu & Soubiran (2025) | MA22=-0.32, MA23f=-0.66, MK24=-0.42, MF24=-0.54 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3297 | 97.2 | 106.98 | -18.93 | 0.11 | -0.36 | 1.69 | – | 0.09 |
