HSC 2170
Summary
HSC 2170 is a poorly populated, very dense object of intermediate 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) | 134.504 | -48.173 | 0.299 | -5.075 | 4.845 | – |
| Cavallo et al. (2024) | 134.506 | -48.16 | 0.3 | – | – | – |
| Hunt & Reffert (2024) | 134.504 | -48.173 | 0.299 | -5.075 | 4.845 | – |
| UCC | 134.509 | -48.164 | 0.304 | -5.065 | 4.841 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=4.738, diffAV50=2.734, MOD50=12.35, logAge50=7.195 |
| Cavallo et al. (2024) | AV50=4.61, dMod50=13.08, logAge50=7.07, [Fe/H]50=0.51 |
| Hunt & Reffert (2024) | MassJ=407.741, MassTot=512.374 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3838 | 92.9 | 134.51 | -48.15 | 0.3 | -5.07 | 4.84 | – | 0.02 |
