HSC 2270
Summary
HSC 2270 is a poorly populated, very loose object of high C3 quality. It is located at a very close distance from the Sun, near 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) | 142.62 | -58.516 | 2.646 | -16.713 | 4.625 | 9.642 |
| Cavallo et al. (2024) | 143.052 | -58.782 | 2.653 | – | – | – |
| UCC | 143.066 | -58.558 | 2.655 | -16.696 | 4.79 | 12.432 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.38, diffAV50=0.733, MOD50=7.801, logAge50=7.67 |
| Cavallo et al. (2024) | AV50=0.53, dMod50=7.87, logAge50=7.52, [Fe/H]50=0.4 |
Search coordinates in Bayestar19
