Ryu 519
Summary
Ryu 519 is a sparse, very dense object of high C3 quality. It is located at a relatively close 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 large percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 265.813 | -30.557 | – | – | – | – |
| UCC | 265.78 | -30.554 | 0.607 | -0.73 | -1.282 | 43.408 |
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 334 | 96.0 | 265.58 | -30.73 | 0.62 | -0.75 | -1.3 | -11.93 | 0.78 |