HSC 1457
Summary
HSC 1457 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, 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) | 60.125 | 6.043 | 1.853 | 0.96 | -7.42 | -0.947 |
| Cavallo et al. (2024) | 60.349 | 6.408 | 1.862 | – | – | – |
| UCC | 60.315 | 6.11 | 1.804 | 1.012 | -7.339 | -1.159 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.371, diffAV50=0.777, MOD50=8.542, logAge50=8.629 |
| Cavallo et al. (2024) | AV50=0.92, dMod50=8.72, logAge50=8.15, [Fe/H]50=-0.01 |
Search coordinates in Bayestar19
