HSC 396
Summary
HSC 396 is a poorly populated, very loose object of very low C3 quality. It is located at a very 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) | 317.192 | -3.671 | 9.723 | 21.795 | -8.722 | -2.508 |
| Cavallo et al. (2024) | 318.352 | -2.796 | 9.805 | – | – | – |
| UCC | 316.85 | -3.279 | 9.652 | 21.088 | -10.347 | -1.181 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.117, diffAV50=0.81, MOD50=4.997, logAge50=8.129 |
| Cavallo et al. (2024) | AV50=0.56, dMod50=5.13, logAge50=8.47, [Fe/H]50=0.05 |
Search coordinates in Bayestar19
