HSC 170
Summary
HSC 170 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) | 301.725 | -28.419 | 3.454 | 2.383 | -14.642 | -14.72 |
| Cavallo et al. (2024) | 301.247 | -27.629 | 3.445 | – | – | – |
| UCC | 299.811 | -27.189 | 3.472 | 2.075 | -14.452 | -15.194 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.175, diffAV50=0.578, MOD50=7.26, logAge50=9.248 |
| Cavallo et al. (2024) | AV50=0.66, dMod50=7.39, logAge50=8.21, [Fe/H]50=-0.02 |
Search coordinates in Bayestar19
