HSC 1708
Summary
HSC 1708 is a sparse, loose object of high C3 quality. It is located at a very 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.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 100.825 | -4.856 | 0.096 | 0.127 | 0.315 | – |
| Hunt & Reffert (2024) | 100.825 | -4.856 | 0.096 | 0.127 | 0.315 | – |
| UCC | 100.82 | -4.855 | 0.087 | 0.127 | 0.337 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.592, diffAV50=1.177, MOD50=14.914, logAge50=8.092 |
| Hunt & Reffert (2024) | MassJ=423.188, MassTot=500.495 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3116 | 80.0 | 100.82 | -4.85 | 0.09 | 0.09 | 0.34 | 95.85 | 0.05 |
