HSC 2452
Summary
HSC 2452 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.
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) | 177.829 | -57.841 | 2.358 | -20.357 | 1.218 | -11.482 |
| Cavallo et al. (2024) | 181.231 | -57.16 | 2.354 | – | – | – |
| UCC | 180.826 | -57.064 | 2.326 | -20.401 | 1.503 | -9.706 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.137, diffAV50=0.775, MOD50=8.065, logAge50=8.189 |
| Cavallo et al. (2024) | AV50=0.5, dMod50=8.12, logAge50=8.13, [Fe/H]50=0.46 |
Search coordinates in Bayestar19
