HSC 2114
Summary
HSC 2114 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a significant 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) | 127.176 | -45.314 | 0.566 | -6.065 | 4.564 | – |
| Cavallo et al. (2024) | 127.564 | -45.289 | 0.569 | – | – | – |
| UCC | 127.352 | -45.262 | 0.569 | -6.033 | 4.61 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.806, diffAV50=1.12, MOD50=11.123, logAge50=7.936 |
| Cavallo et al. (2024) | AV50=1.52, dMod50=11.28, logAge50=7.83, [Fe/H]50=0.34 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 4130 | 72.0 | 127.52 | -45.3 | 0.56 | -6.06 | 4.58 | – | 0.03 |
