HSC 390
Summary
HSC 390 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, below 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) | 317.153 | -4.506 | 2.558 | 7.379 | 1.442 | -19.264 |
| Cavallo et al. (2024) | 316.532 | -4.075 | 2.554 | – | – | – |
| UCC | 316.823 | -3.693 | 2.554 | 7.327 | 1.362 | -8.376 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.279, diffAV50=0.53, MOD50=7.884, logAge50=7.951 |
| Cavallo et al. (2024) | AV50=0.57, dMod50=8.08, logAge50=8.3, [Fe/H]50=0.06 |
Search coordinates in Bayestar19
