HSC 1722
Summary
HSC 1722 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 104.541 | -4.754 | 0.428 | -1.769 | 0.756 | – |
| Cavallo et al. (2024) | 104.593 | -4.727 | 0.426 | – | – | – |
| Hunt & Reffert (2024) | 104.541 | -4.754 | 0.428 | -1.769 | 0.756 | – |
| UCC | 104.568 | -4.75 | 0.429 | -1.758 | 0.754 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.19, diffAV50=2.078, MOD50=11.609, logAge50=7.76 |
| Cavallo et al. (2024) | AV50=1.18, dMod50=11.52, logAge50=7.9, [Fe/H]50=0.15 |
| Hunt & Reffert (2024) | MassJ=351.034, MassTot=351.034 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Collinder 123 | 4.4 | 104.45 | -4.61 | 0.45 | -1.31 | 1.0 | 32.11 | 0.9 |
