CWNU 1018
Summary
CWNU 1018 is a poorly populated, very dense object of high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 69.129 | -8.632 | 6.055 | -9.469 | -4.717 | – |
| Hunt & Reffert (2023) | 68.621 | -8.431 | 5.938 | -9.856 | -4.139 | 17.555 |
| Cavallo et al. (2024) | 70.274 | -9.564 | 5.955 | – | – | – |
| UCC | 68.677 | -8.596 | 6.051 | -9.447 | -4.648 | 20.404 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.35, logAge=8.15 |
| Hunt & Reffert (2023) | AV50=0.03, diffAV50=0.262, MOD50=6.105, logAge50=8.186 |
| Cavallo et al. (2024) | AV50=0.37, dMod50=6.17, logAge50=8.13, [Fe/H]50=0.27 |
Search coordinates in Bayestar19
