HSC 1812
Summary
HSC 1812 is a sparse, very loose object of very 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) | 111.049 | -14.427 | 0.241 | -0.843 | 0.161 | – |
| Cavallo et al. (2024) | 111.093 | -14.464 | 0.239 | – | – | – |
| Hunt & Reffert (2024) | 111.049 | -14.427 | 0.241 | -0.843 | 0.161 | – |
| UCC | 111.094 | -14.459 | 0.23 | -0.836 | 0.065 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.725, diffAV50=0.99, MOD50=12.752, logAge50=8.503 |
| Cavallo et al. (2024) | AV50=1.7, dMod50=12.33, logAge50=8.44, [Fe/H]50=-0.4 |
| Hunt & Reffert (2024) | MassJ=146.672, MassTot=291.198 |
Search coordinates in Bayestar19
