HSC 2590
Summary
HSC 2590 is a sparse, loose object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) | 201.979 | -61.879 | 0.776 | -4.911 | -3.068 | 6.418 |
| Cavallo et al. (2024) | 202.058 | -61.855 | 0.78 | – | – | – |
| Hunt & Reffert (2024) | 201.979 | -61.879 | 0.776 | -4.911 | -3.068 | 6.418 |
| UCC | 201.984 | -61.874 | 0.766 | -4.894 | -3.05 | 3.725 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.954, diffAV50=0.648, MOD50=10.476, logAge50=8.086 |
| Cavallo et al. (2024) | AV50=0.64, dMod50=10.48, logAge50=8.31, [Fe/H]50=0.38 |
| Hunt & Reffert (2024) | MassJ=107.016, MassTot=126.596 |
Search coordinates in Bayestar19