CWNU 89
Summary
CWNU 89 is a poorly populated, moderately dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 133.295 | -54.428 | 0.78 | -5.68 | 4.48 | – |
| Hunt & Reffert (2023) | 133.141 | -54.446 | 0.779 | -5.692 | 4.513 | 16.56 |
| Cavallo et al. (2024) | 133.211 | -54.461 | 0.783 | – | – | – |
| Hunt & Reffert (2024) | 133.141 | -54.446 | 0.779 | -5.692 | 4.513 | 16.56 |
| UCC | 133.239 | -54.426 | 0.777 | -5.717 | 4.455 | 13.666 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.45, m-M=10.45, logAge=7.9, Z=0.02 |
| Hunt & Reffert (2023) | AV50=0.319, diffAV50=0.238, MOD50=10.396, logAge50=7.735 |
| Cavallo et al. (2024) | AV50=0.11, dMod50=10.32, logAge50=8.25, [Fe/H]50=0.49 |
| Hunt & Reffert (2024) | MassJ=77.4245, MassTot=85.1406 |
Search coordinates in Bayestar19
