HSC 295
Summary
HSC 295 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) | 273.828 | 1.019 | 2.542 | -1.357 | -13.352 | -15.187 |
| Cavallo et al. (2024) | 273.741 | 1.56 | 2.557 | – | – | – |
| UCC | 273.88 | 0.977 | 2.569 | -1.261 | -13.683 | -15.472 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.081, diffAV50=1.646, MOD50=7.848, logAge50=8.187 |
| Cavallo et al. (2024) | AV50=1.19, dMod50=8.0, logAge50=8.42, [Fe/H]50=0.48 |
Search coordinates in Bayestar19
