Ryu 419
Summary
Ryu 419 is a poorly populated, very loose object of low 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) | 258.187 | -36.637 | – | – | – | – |
| UCC | 258.176 | -36.649 | 0.151 | -3.936 | -6.016 | 6.195 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19