CWNU 2018
Summary
CWNU 2018 is a sparse, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 354.371 | 58.375 | 0.393 | -0.007 | -0.792 | – |
| Hunt & Reffert (2023) | 354.301 | 58.372 | 0.387 | -0.058 | -0.776 | -43.378 |
| Cavallo et al. (2024) | 354.328 | 58.409 | 0.389 | – | – | – |
| Hunt & Reffert (2024) | 354.301 | 58.372 | 0.387 | -0.058 | -0.776 | -43.378 |
| UCC | 354.352 | 58.375 | 0.389 | -0.007 | -0.78 | -44.48 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.05, m-M=11.9, logAge=6.35 |
| Hunt & Reffert (2023) | AV50=2.092, diffAV50=0.862, MOD50=11.926, logAge50=8.182 |
| Cavallo et al. (2024) | AV50=2.15, dMod50=11.88, logAge50=8.34, [Fe/H]50=0.29 |
| Hunt & Reffert (2024) | MassJ=106.495, MassTot=212.234 |
Search coordinates in Bayestar19
