HSC 2278
Summary
HSC 2278 is a poorly populated, very loose object of 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) | 172.153 | -24.589 | 7.976 | -9.356 | 0.728 | 1.308 |
| Cavallo et al. (2024) | 169.663 | -23.463 | 7.944 | – | – | – |
| Hu & Soubiran (2025) | 169.663 | -23.463 | – | – | – | – |
| UCC | 169.079 | -25.051 | 7.861 | -9.271 | 0.677 | 2.209 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.092, diffAV50=0.288, MOD50=5.389, logAge50=8.756 |
| Cavallo et al. (2024) | AV50=0.44, dMod50=5.55, logAge50=9.18, [Fe/H]50=0.08 |
| Hu & Soubiran (2025) | MA22=-0.26, MA23f=-0.33, MZ23=-0.07, MK24=-0.09, MF24=-0.5 |
Search coordinates in Bayestar19
