CWNU 124
Summary
CWNU 124 is a sparse, very dense object of low C3 quality. It is located at a close distance from the Sun, above 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) | 349.121 | 64.689 | 1.0 | 0.63 | -0.46 | – |
| Hunt & Reffert (2023) | 349.21 | 64.694 | 1.0 | 0.623 | -0.443 | -20.639 |
| Cavallo et al. (2024) | 349.177 | 64.671 | 0.999 | – | – | – |
| Hunt & Reffert (2024) | 349.21 | 64.694 | 1.0 | 0.623 | -0.443 | -20.639 |
| UCC | 349.188 | 64.718 | 1.001 | 0.626 | -0.457 | -33.512 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=1.85, m-M=10.4, logAge=8.2, Z=0.03 |
| Hunt & Reffert (2023) | AV50=2.101, diffAV50=0.485, MOD50=10.065, logAge50=8.362 |
| Cavallo et al. (2024) | AV50=1.84, dMod50=10.08, logAge50=8.21, [Fe/H]50=0.41 |
| Hunt & Reffert (2024) | MassJ=86.5561, MassTot=98.1461 |
Search coordinates in Bayestar19
