Ryu 513
Summary
Ryu 513 is a poorly populated, 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 very small percentage of members with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 265.823 | -31.667 | – | – | – | – |
| UCC | 265.827 | -31.661 | 0.413 | -0.896 | -1.8 | -0.589 |
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 |
|---|---|---|---|---|---|---|---|---|
| VVV 139 | 6.2 | 265.93 | -31.68 | 0.5 | -0.63 | -0.97 | -28.78 | 0.09 |
| VVV 140 | 6.2 | 265.95 | -31.68 | 0.5 | -0.68 | -0.96 | -28.78 | 0.05 |