HSC 1790
Summary
HSC 1790 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) | 107.212 | -13.739 | 0.398 | -2.405 | -0.433 | – |
| Hunt & Reffert (2024) | 107.212 | -13.739 | 0.398 | -2.405 | -0.433 | – |
| UCC | 107.214 | -13.736 | 0.412 | -2.416 | -0.426 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.602, diffAV50=1.068, MOD50=11.778, logAge50=8.485 |
| Hunt & Reffert (2024) | MassJ=132.946, MassTot=116.413 |
Search coordinates in Bayestar19
