HSC 1797
Summary
HSC 1797 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) | 108.779 | -13.768 | 0.694 | -2.441 | 1.586 | – |
| Hunt & Reffert (2024) | 108.779 | -13.768 | 0.694 | -2.441 | 1.586 | – |
| UCC | 108.795 | -13.745 | 0.692 | -2.438 | 1.558 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.693, diffAV50=0.343, MOD50=10.678, logAge50=8.371 |
| Hunt & Reffert (2024) | MassJ=81.7617, MassTot=66.8812 |
Search coordinates in Bayestar19
