HSC 1292
Summary
HSC 1292 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively 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) | 78.281 | 42.282 | 0.888 | -0.104 | -4.01 | 6.91 |
| Cavallo et al. (2024) | 78.304 | 41.965 | 0.897 | – | – | – |
| UCC | 78.293 | 42.109 | 0.895 | -0.114 | -4.063 | 3.996 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.511, diffAV50=0.438, MOD50=10.145, logAge50=8.14 |
| Cavallo et al. (2024) | AV50=1.0, dMod50=10.31, logAge50=7.52, [Fe/H]50=-0.1 |
Search coordinates in Bayestar19