HSC 1190
Summary
HSC 1190 is a sparse, very loose object of low C3 quality. It is located at a large 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) | 62.952 | 54.316 | 0.162 | -0.191 | -0.143 | – |
| Cavallo et al. (2024) | 62.863 | 54.38 | 0.161 | – | – | – |
| Hunt & Reffert (2024) | 62.952 | 54.316 | 0.162 | -0.191 | -0.143 | – |
| UCC | 62.889 | 54.32 | 0.152 | -0.21 | -0.132 | -37.01 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.635, diffAV50=2.472, MOD50=13.622, logAge50=7.204 |
| Cavallo et al. (2024) | AV50=3.27, dMod50=13.31, logAge50=7.45, [Fe/H]50=0.6 |
| Hunt & Reffert (2024) | MassJ=269.680, MassTot=683.450 |
Search coordinates in Bayestar19