Ryu 814
Summary
Ryu 814 is a sparse, very loose object of 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) | 276.464 | -9.114 | – | – | – | – |
| UCC | 276.467 | -9.113 | 0.227 | -2.32 | -4.311 | 33.872 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19