HSC 1137
Summary
HSC 1137 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, above 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) | 181.59 | 48.722 | 4.994 | 13.212 | 0.895 | -10.774 |
| Cavallo et al. (2024) | 179.302 | 48.937 | 5.03 | – | – | – |
| UCC | 177.536 | 46.9 | 5.067 | 11.516 | 0.936 | -10.398 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.119, diffAV50=0.321, MOD50=6.539, logAge50=8.369 |
| Cavallo et al. (2024) | AV50=0.43, dMod50=6.56, logAge50=8.4, [Fe/H]50=0.1 |
Search coordinates in Bayestar19
