CWNU 1832
Summary
CWNU 1832 is a poorly populated, dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 257.695 | -36.015 | 0.581 | 1.366 | 0.443 | -29.44 |
| Hunt & Reffert (2023) | 257.692 | -36.029 | 0.561 | 1.334 | 0.408 | -29.454 |
| Cavallo et al. (2024) | 257.683 | -36.023 | 0.569 | – | – | – |
| Hunt & Reffert (2024) | 257.692 | -36.029 | 0.561 | 1.334 | 0.408 | -29.454 |
| UCC | 257.689 | -36.028 | 0.567 | 1.348 | 0.441 | -29.438 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.65, m-M=11.1, logAge=8.15 |
| Hunt & Reffert (2023) | AV50=3.436, diffAV50=2.166, MOD50=11.09, logAge50=7.982 |
| Cavallo et al. (2024) | AV50=3.65, dMod50=11.0, logAge50=8.09, [Fe/H]50=-0.33 |
| Hunt & Reffert (2024) | MassJ=400.383, MassTot=409.432 |
Search coordinates in Bayestar19
