HSC 2297
Summary
HSC 2297 is a poorly populated, very loose object of 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) | 132.296 | -65.561 | 2.263 | -4.008 | 8.288 | 13.791 |
| Cavallo et al. (2024) | 133.628 | -63.553 | 2.257 | – | – | – |
| UCC | 133.318 | -62.834 | 2.23 | -3.997 | 8.307 | 20.697 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.543, diffAV50=1.187, MOD50=8.14, logAge50=7.984 |
| Cavallo et al. (2024) | AV50=0.74, dMod50=8.35, logAge50=7.74, [Fe/H]50=-0.11 |
Search coordinates in Bayestar19
