CWNU 2890
Summary
CWNU 2890 is a sparse, very dense object of intermediate 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) | 262.41 | -34.314 | 0.614 | 1.968 | 0.218 | – |
| Hunt & Reffert (2023) | 262.423 | -34.321 | 0.599 | 1.873 | 0.176 | 112.443 |
| Cavallo et al. (2024) | 262.387 | -34.321 | 0.597 | – | – | – |
| Hunt & Reffert (2024) | 262.423 | -34.321 | 0.599 | 1.873 | 0.176 | 112.443 |
| UCC | 262.398 | -34.329 | 0.606 | 1.976 | 0.163 | 112.425 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=4.6, m-M=10.9, logAge=8.2 |
| Hunt & Reffert (2023) | AV50=4.074, diffAV50=2.547, MOD50=10.989, logAge50=7.477 |
| Cavallo et al. (2024) | AV50=4.37, dMod50=11.35, logAge50=8.15, [Fe/H]50=-0.3 |
| Hunt & Reffert (2024) | MassJ=296.762, MassTot=317.250 |
Search coordinates in Bayestar19
