HSC 2251
Summary
HSC 2251 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.79) 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) | 154.881 | -45.523 | 2.429 | -0.591 | -0.173 | -8.222 |
| Cavallo et al. (2024) | 151.251 | -44.276 | 2.432 | – | – | – |
| UCC | 151.208 | -44.023 | 2.441 | -0.694 | -0.108 | -8.052 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.086, diffAV50=0.287, MOD50=7.925, logAge50=8.728 |
| Cavallo et al. (2024) | AV50=0.34, dMod50=8.09, logAge50=8.35, [Fe/H]50=0.05 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 1161 | 20.7 | 154.49 | -45.44 | 2.53 | -0.27 | -0.55 | -9.07 | 0.07 |
