HSC 52
Summary
HSC 52 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
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) | 336.342 | -38.019 | 4.072 | 17.431 | 0.086 | -6.633 |
| Cavallo et al. (2024) | 337.078 | -38.789 | 4.068 | – | – | – |
| UCC | 336.578 | -38.16 | 4.015 | 17.294 | -0.034 | -3.475 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.038, diffAV50=0.315, MOD50=6.944, logAge50=8.299 |
| Cavallo et al. (2024) | AV50=0.4, dMod50=7.0, logAge50=8.18, [Fe/H]50=0.16 |
Search coordinates in Bayestar19
