HSC 927
Summary
HSC 927 is a sparse, very loose object of very low C3 quality. It is located at a close distance from the Sun, above 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) | 353.828 | 70.09 | 1.672 | -8.288 | -3.676 | -5.691 |
| Cavallo et al. (2024) | 350.873 | 69.764 | 1.672 | – | – | – |
| Hu & Soubiran (2025) | 350.873 | 69.764 | – | – | – | – |
| UCC | 350.383 | 69.561 | 1.627 | -8.3 | -3.771 | -21.899 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.537, diffAV50=1.255, MOD50=8.789, logAge50=9.031 |
| Cavallo et al. (2024) | AV50=1.49, dMod50=8.98, logAge50=9.1, [Fe/H]50=0.38 |
| Hu & Soubiran (2025) | MA22=0.02, MA23f=-0.09, MK24=-0.09, MF24=-0.05 |
Search coordinates in Bayestar19