CWNU 42
Summary
CWNU 42 is a sparse, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, near 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. (2022) | 318.251 | 46.07 | 0.41 | 0.06 | -1.64 | – |
| Hunt & Reffert (2023) | 318.273 | 46.083 | 0.398 | 0.018 | -1.699 | -11.411 |
| Cavallo et al. (2024) | 318.241 | 46.052 | 0.4 | – | – | – |
| Hunt & Reffert (2024) | 318.273 | 46.083 | 0.398 | 0.018 | -1.699 | -11.411 |
| UCC | 318.276 | 46.068 | 0.408 | 0.062 | -1.674 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=1.3, m-M=11.7, logAge=7.5, Z=0.02 |
| Hunt & Reffert (2023) | AV50=1.444, diffAV50=2.47, MOD50=11.813, logAge50=8.431 |
| Cavallo et al. (2024) | AV50=1.66, dMod50=11.9, logAge50=8.25, [Fe/H]50=-0.05 |
| Hunt & Reffert (2024) | MassJ=255.831, MassTot=391.790 |
Search coordinates in Bayestar19
