Ryu 357
Summary
Ryu 357 is a poorly populated, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
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 |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 251.679 | -41.874 | – | – | – | – |
| UCC | 251.689 | -41.868 | 0.137 | -4.749 | -5.734 | -46.519 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19