CWNU 1730
Summary
CWNU 1730 is a poorly populated, very dense object of intermediate 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. (2023) | 164.68 | -60.127 | 0.385 | -6.143 | 0.818 | – |
| Hunt & Reffert (2023) | 164.698 | -60.119 | 0.389 | -6.132 | 0.819 | – |
| Cavallo et al. (2024) | 164.678 | -60.122 | 0.385 | – | – | – |
| Hunt & Reffert (2024) | 164.698 | -60.119 | 0.389 | -6.132 | 0.819 | – |
| UCC | 164.687 | -60.125 | 0.389 | -6.142 | 0.813 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.35, m-M=11.9, logAge=8.0 |
| Hunt & Reffert (2023) | AV50=0.896, diffAV50=0.775, MOD50=11.88, logAge50=8.166 |
| Cavallo et al. (2024) | AV50=1.45, dMod50=11.74, logAge50=7.93, [Fe/H]50=-0.42 |
| Hunt & Reffert (2024) | MassJ=181.888, MassTot=202.399 |
Search coordinates in Bayestar19
