Ryu 089
Summary
Ryu 089 is a poorly populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 253.245 | -41.676 | – | – | – | – |
| Hunt & Reffert (2023) | 253.244 | -41.679 | 0.344 | -0.806 | -2.948 | -26.815 |
| Cavallo et al. (2024) | 253.233 | -41.662 | 0.341 | – | – | – |
| Hunt & Reffert (2024) | 253.244 | -41.679 | 0.344 | -0.806 | -2.948 | -26.815 |
| UCC | 253.246 | -41.678 | 0.354 | -0.807 | -2.954 | -28.437 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=4.502, diffAV50=2.881, MOD50=12.098, logAge50=8.362 |
| Cavallo et al. (2024) | AV50=4.67, dMod50=12.79, logAge50=7.78, [Fe/H]50=0.67 |
| Hunt & Reffert (2024) | MassJ=3144.74, MassTot=3144.74 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3138 | 100.0 | 253.25 | -41.67 | 0.35 | -0.81 | -2.94 | -27.9 | 0.43 |
