CWNU 1994
Summary
CWNU 1994 is a sparse, very dense object of high C3 quality. It is located at a relatively close 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. (2023) | 278.682 | -11.602 | 0.506 | 0.334 | -0.1 | – |
| Hunt & Reffert (2023) | 278.692 | -11.626 | 0.514 | 0.268 | -0.179 | 6.108 |
| Cavallo et al. (2024) | 278.656 | -11.605 | 0.513 | – | – | – |
| Hunt & Reffert (2024) | 278.692 | -11.626 | 0.514 | 0.268 | -0.179 | 6.108 |
| UCC | 278.687 | -11.573 | 0.506 | 0.313 | -0.125 | 6.109 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.3, m-M=11.3, logAge=6.65 |
| Hunt & Reffert (2023) | AV50=2.52, diffAV50=1.252, MOD50=11.31, logAge50=8.223 |
| Cavallo et al. (2024) | AV50=2.54, dMod50=11.0, logAge50=8.03, [Fe/H]50=-0.05 |
| Hunt & Reffert (2024) | MassJ=173.028, MassTot=173.028 |
Search coordinates in Bayestar19
