HSC 1726
Summary
HSC 1726 is a poorly populated, very dense object of very high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a very small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 101.881 | -6.381 | 0.091 | -0.288 | 0.503 | – |
| Cavallo et al. (2024) | 101.867 | -6.286 | 0.091 | – | – | – |
| Hunt & Reffert (2024) | 101.881 | -6.381 | 0.091 | -0.288 | 0.503 | – |
| UCC | 101.879 | -6.38 | 0.131 | -0.365 | 0.529 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.242, diffAV50=1.072, MOD50=14.573, logAge50=7.919 |
| Cavallo et al. (2024) | AV50=1.08, dMod50=13.41, logAge50=8.09, [Fe/H]50=0.11 |
| Hunt & Reffert (2024) | MassJ=215.436, MassTot=788.591 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4028 | 7.1 | 102.0 | -6.3 | 0.11 | -0.19 | 0.56 | 61.53 | 0.07 |
