HSC 957
Summary
HSC 957 is a sparse, very loose object of low C3 quality. It is located at a 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) | 8.878 | 49.44 | 1.246 | -1.567 | -4.273 | -19.664 |
| Cavallo et al. (2024) | 8.48 | 49.322 | 1.259 | – | – | – |
| UCC | 8.735 | 49.416 | 1.257 | -1.564 | -4.282 | -16.732 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.313, diffAV50=0.493, MOD50=9.407, logAge50=8.185 |
| Cavallo et al. (2024) | AV50=0.54, dMod50=9.64, logAge50=8.64, [Fe/H]50=-0.08 |
Search coordinates in Bayestar19
