HSC 2298
Summary
HSC 2298 is a poorly populated, loose object of intermediate C3 quality. It is located at a close distance from the Sun, near 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) | 145.729 | -60.392 | 1.573 | -9.742 | 6.889 | 6.572 |
| Cavallo et al. (2024) | 146.453 | -60.668 | 1.578 | – | – | – |
| UCC | 145.753 | -60.373 | 1.587 | -9.656 | 6.975 | 7.301 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.207, diffAV50=0.344, MOD50=8.896, logAge50=8.003 |
| Cavallo et al. (2024) | AV50=0.51, dMod50=9.01, logAge50=8.0, [Fe/H]50=0.09 |
Search coordinates in Bayestar19
