HSC 1799
Summary
HSC 1799 is a sparse, loose object of low C3 quality. It is located at a moderate 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) | 112.969 | -11.747 | 0.479 | -2.771 | 2.67 | 27.483 |
| Cavallo et al. (2024) | 112.994 | -11.788 | 0.479 | – | – | – |
| Hunt & Reffert (2024) | 112.969 | -11.747 | 0.479 | -2.771 | 2.67 | 27.483 |
| UCC | 112.992 | -11.788 | 0.477 | -2.796 | 2.666 | 27.472 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.148, diffAV50=0.251, MOD50=11.441, logAge50=8.152 |
| Cavallo et al. (2024) | AV50=0.48, dMod50=11.42, logAge50=8.32, [Fe/H]50=-0.32 |
| Hunt & Reffert (2024) | MassJ=64.1355, MassTot=94.2806 |
Search coordinates in Bayestar19
