HSC 1234
Summary
HSC 1234 is a sparse, very loose object of very low C3 quality. It is located at a very close distance from the Sun, near 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) | 58.5 | 40.44 | 2.525 | -0.149 | -10.328 | 2.759 |
| Cavallo et al. (2024) | 58.586 | 41.065 | 2.519 | – | – | – |
| Hu & Soubiran (2025) | 58.586 | 41.065 | – | – | – | – |
| UCC | 58.665 | 41.404 | 2.502 | -0.171 | -10.242 | 4.163 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.414, diffAV50=0.253, MOD50=7.846, logAge50=9.783 |
| Cavallo et al. (2024) | AV50=0.72, dMod50=8.07, logAge50=8.98, [Fe/H]50=0.21 |
| Hu & Soubiran (2025) | MA22=-0.25, MA23f=-0.07, MZ23=-0.05, MK24=-0.01, MF24=-0.15 |
Search coordinates in Bayestar19