Ryu 210
Summary
Ryu 210 is a sparse, very dense object of very low 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 is likely a unique object, which shares a moderate percentage of members with at least one previously 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) | 274.325 | -16.933 | – | – | – | – |
| UCC | 274.312 | -16.911 | 0.56 | -0.784 | -2.229 | 13.88 |
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 |
|---|---|---|---|---|---|---|---|---|
| VVVX CL093 | 32.0 | 274.38 | -16.97 | 0.61 | -1.54 | -3.1 | 4.2 | 0.42 |
| VVVX CL095 | 16.0 | 274.4 | -16.93 | 0.52 | -0.27 | -2.16 | -11.4 | 0.05 |
| VVVX CL092 | 12.0 | 274.26 | -17.08 | 0.56 | -1.18 | -2.63 | – | 0.1 |
| VVVX CL087 | 4.0 | 274.07 | -16.87 | 0.44 | -1.13 | -2.19 | – | 0.07 |