CWNU 264
Summary
CWNU 264 is a sparse, very dense object of intermediate C3 quality. It is located at a relatively close 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. (2022) | 149.21 | -60.52 | 0.76 | -9.28 | 3.69 | – |
| Hunt & Reffert (2023) | 149.2 | -60.53 | 0.767 | -9.321 | 3.647 | -22.985 |
| Cavallo et al. (2024) | 149.216 | -60.512 | 0.765 | – | – | – |
| Hunt & Reffert (2024) | 149.2 | -60.53 | 0.767 | -9.321 | 3.647 | -22.985 |
| UCC | 149.183 | -60.521 | 0.765 | -9.293 | 3.649 | -13.618 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.3, m-M=10.2, logAge=7.6, Z=0.01 |
| Hunt & Reffert (2023) | AV50=0.314, diffAV50=0.395, MOD50=10.504, logAge50=7.681 |
| Cavallo et al. (2024) | AV50=0.32, dMod50=10.27, logAge50=8.03, [Fe/H]50=-0.38 |
| Hunt & Reffert (2024) | MassJ=42.6544, MassTot=84.1774 |
Search coordinates in Bayestar19
