Ryu 148
Summary
Ryu 148 is a sparse, very dense object of 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) | 267.308 | -31.395 | – | – | – | – |
| UCC | 267.323 | -31.397 | 0.739 | -1.168 | -2.212 | -38.161 |
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 |
|---|---|---|---|---|---|---|---|---|
| Dutra Bica 51 | 32.0 | 267.38 | -31.27 | 0.73 | -1.12 | -2.09 | -5.21 | 0.69 |