Ryu 534
Summary
Ryu 534 is a sparse, very dense object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a significant percentage of members with 3 later reported entries.
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) | 266.361 | -29.076 | – | – | – | – |
| UCC | 266.383 | -29.081 | 0.5 | 1.784 | -0.82 | -36.722 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 335 | 68.0 | 266.57 | -29.18 | 0.48 | 1.72 | -0.79 | -34.64 | 0.27 |
| CWWDL 1660 | 20.0 | 266.57 | -29.17 | 0.48 | 1.7 | -0.8 | -34.92 | 0.0 |
| FoF 1624 | 20.0 | 266.58 | -29.17 | 0.48 | 1.72 | -0.79 | -34.94 | 0.68 |