CWNU 1722
Summary
CWNU 1722 is a poorly populated, moderately dense object of low C3 quality. It is located at a moderate 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. (2023) | 8.73 | 60.605 | 0.287 | -1.596 | -0.906 | – |
| Hunt & Reffert (2023) | 8.753 | 60.566 | 0.272 | -1.623 | -0.887 | -44.389 |
| Cavallo et al. (2024) | 8.727 | 60.59 | 0.275 | – | – | – |
| Hunt & Reffert (2024) | 8.753 | 60.566 | 0.272 | -1.623 | -0.887 | -44.389 |
| UCC | 8.743 | 60.595 | 0.287 | -1.614 | -0.903 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.4, m-M=12.9, logAge=7.45 |
| Hunt & Reffert (2023) | AV50=1.816, diffAV50=2.23, MOD50=12.603, logAge50=8.351 |
| Cavallo et al. (2024) | AV50=1.64, dMod50=12.75, logAge50=8.37, [Fe/H]50=0.51 |
| Hunt & Reffert (2024) | MassJ=320.276, MassTot=416.758 |
Search coordinates in Bayestar19
