CWNU 488
Summary
CWNU 488 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 269.574 | -25.272 | 0.38 | 0.31 | -1.42 | – |
| Hunt & Reffert (2023) | 269.568 | -25.258 | 0.392 | 0.291 | -1.422 | – |
| Cavallo et al. (2024) | 269.57 | -25.265 | 0.391 | – | – | – |
| Hunt & Reffert (2024) | 269.568 | -25.258 | 0.392 | 0.291 | -1.422 | – |
| UCC | 269.571 | -25.255 | 0.397 | 0.307 | -1.416 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=2.7, m-M=12.85, logAge=6.7, Z=0.03 |
| Hunt & Reffert (2023) | AV50=2.096, diffAV50=2.003, MOD50=11.802, logAge50=8.079 |
| Cavallo et al. (2024) | AV50=2.81, dMod50=13.54, logAge50=7.66, [Fe/H]50=-2.02 |
| Hunt & Reffert (2024) | MassJ=396.843, MassTot=396.843 |
Search coordinates in Bayestar19
