Ryu 288
Summary
Ryu 288 is a sparse, very dense object of 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 large percentage of members with 2 later reported entries.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 243.735 | -51.63 | – | – | – | – |
| UCC | 243.743 | -51.652 | 0.366 | -3.609 | -3.991 | -34.76 |
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 |
|---|---|---|---|---|---|---|---|---|
| CWWDL 1583 | 80.0 | 243.74 | -51.69 | 0.35 | -3.61 | -4.01 | -34.39 | 0.15 |
| UBC 540 | 56.0 | 243.76 | -51.69 | 0.33 | -3.58 | -4.02 | -34.76 | 0.42 |