Ryu 52
Summary
Ryu 52 is a sparse, loose object of very low C3 quality. It is located at a moderate 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: 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 |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 246.386 | -46.937 | – | – | – | – |
| UCC | 246.387 | -46.941 | 0.203 | -5.026 | -5.25 | – |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19