HSC 1817
Summary
HSC 1817 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) | 109.487 | -16.288 | 0.226 | -1.096 | 1.276 | 107.146 |
| Cavallo et al. (2024) | 109.493 | -16.293 | 0.228 | – | – | – |
| Hunt & Reffert (2024) | 109.487 | -16.288 | 0.226 | -1.096 | 1.276 | 107.146 |
| UCC | 109.495 | -16.287 | 0.218 | -1.113 | 1.296 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.776, diffAV50=2.576, MOD50=12.594, logAge50=8.176 |
| Cavallo et al. (2024) | AV50=1.78, dMod50=13.13, logAge50=8.58, [Fe/H]50=0.58 |
| Hunt & Reffert (2024) | MassJ=282.896, MassTot=350.698 |
Search coordinates in Bayestar19
