HSC 392
Summary
HSC 392 is a sparse, very loose object of low C3 quality. It is located at a moderate 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) | 294.929 | 8.268 | 0.476 | -0.666 | -5.283 | – |
| Hunt & Reffert (2024) | 294.929 | 8.268 | 0.476 | -0.666 | -5.283 | – |
| UCC | 294.964 | 8.256 | 0.451 | -0.703 | -5.279 | -26.411 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.666, diffAV50=1.037, MOD50=11.514, logAge50=9.899 |
| Hunt & Reffert (2024) | MassJ=279.911, MassTot=154.775 |
Search coordinates in Bayestar19
