HSC 1270
Summary
HSC 1270 is a sparse, very loose object of very low C3 quality. It is located at a close distance from the Sun, near 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) | 67.897 | 41.228 | 1.819 | 7.848 | -10.861 | 5.42 |
| Cavallo et al. (2024) | 66.712 | 42.429 | 1.822 | – | – | – |
| UCC | 67.195 | 42.01 | 1.829 | 7.957 | -10.931 | 9.675 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.022, diffAV50=0.974, MOD50=8.603, logAge50=7.991 |
| Cavallo et al. (2024) | AV50=1.11, dMod50=8.72, logAge50=8.47, [Fe/H]50=0.48 |
Search coordinates in Bayestar19
