HSC 1070
Summary
HSC 1070 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above 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) | 33.438 | 64.893 | 0.293 | -0.164 | 0.222 | – |
| Cavallo et al. (2024) | 33.48 | 64.909 | 0.296 | – | – | – |
| Hunt & Reffert (2024) | 33.438 | 64.893 | 0.293 | -0.164 | 0.222 | – |
| UCC | 33.492 | 64.898 | 0.279 | -0.155 | 0.235 | -65.849 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=2.088, diffAV50=1.036, MOD50=12.513, logAge50=8.655 |
| Cavallo et al. (2024) | AV50=2.5, dMod50=12.95, logAge50=8.22, [Fe/H]50=0.18 |
| Hunt & Reffert (2024) | MassJ=237.957, MassTot=287.177 |
Search coordinates in Bayestar19