HSC 2609
Summary
HSC 2609 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
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) | 223.64 | -78.133 | 2.754 | -10.792 | -9.664 | 11.678 |
| Cavallo et al. (2024) | 228.341 | -77.071 | 2.749 | – | – | – |
| UCC | 228.836 | -77.566 | 2.773 | -11.029 | -9.973 | 2.687 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.253, diffAV50=0.477, MOD50=7.718, logAge50=8.033 |
| Cavallo et al. (2024) | AV50=0.6, dMod50=7.89, logAge50=8.1, [Fe/H]50=-0.1 |
Search coordinates in Bayestar19
