HSC 1570
Summary
HSC 1570 is a sparse, very loose object of intermediate 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 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) | 94.765 | 12.876 | 0.156 | 0.188 | -0.23 | 46.345 |
| Cavallo et al. (2024) | 94.816 | 12.789 | 0.16 | – | – | – |
| Hunt & Reffert (2024) | 94.765 | 12.876 | 0.156 | 0.188 | -0.23 | 46.345 |
| UCC | 94.78 | 12.89 | 0.174 | 0.122 | -0.301 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.322, diffAV50=2.173, MOD50=13.515, logAge50=8.293 |
| Cavallo et al. (2024) | AV50=2.51, dMod50=13.35, logAge50=8.4, [Fe/H]50=0.07 |
| Hunt & Reffert (2024) | MassJ=592.459, MassTot=1257.69 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3957 | 84.0 | 94.78 | 12.88 | 0.17 | 0.1 | -0.33 | – | 0.03 |
