Ryu 54
Summary
Ryu 54 is a poorly populated, very loose object of very low C3 quality. It is located at a very large distance from the Sun, well below 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) | 250.271 | -49.061 | – | – | – | – |
| UCC | 250.228 | -49.051 | 0.029 | -3.361 | -4.895 | – |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19