HSC 1067
Summary
HSC 1067 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) | 33.367 | 65.447 | 1.412 | -5.543 | -1.23 | -12.892 |
| Cavallo et al. (2024) | 32.217 | 65.003 | 1.408 | – | – | – |
| UCC | 33.366 | 65.223 | 1.399 | -5.564 | -1.235 | -26.628 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.357, diffAV50=0.923, MOD50=9.138, logAge50=8.342 |
| Cavallo et al. (2024) | AV50=0.74, dMod50=9.32, logAge50=8.22, [Fe/H]50=0.7 |
Search coordinates in Bayestar19
