HSC 1675
Summary
HSC 1675 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 94.531 | -3.341 | 0.156 | 0.052 | 0.212 | 116.811 |
| Cavallo et al. (2024) | 94.573 | -3.44 | 0.158 | – | – | – |
| UCC | 94.577 | -3.376 | 0.162 | 0.059 | 0.213 | 96.547 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.345, diffAV50=1.423, MOD50=13.589, logAge50=8.89 |
| Cavallo et al. (2024) | AV50=0.21, dMod50=13.27, logAge50=9.11, [Fe/H]50=-0.13 |
Search coordinates in Bayestar19
