Ryu 614
Summary
Ryu 614 is a poorly populated, very loose object of low C3 quality. It is located at a very large distance from the Sun, 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) | 273.058 | -23.567 | – | – | – | – |
| UCC | 273.067 | -23.566 | 0.095 | -4.459 | -7.312 | – |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19