CWNU 2006
Summary
CWNU 2006 is a sparse, loose 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.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 113.646 | -17.144 | 0.606 | -3.251 | 0.986 | – |
| Hunt & Reffert (2023) | 113.581 | -17.187 | 0.608 | -3.271 | 1.009 | – |
| Cavallo et al. (2024) | 113.612 | -17.141 | 0.608 | – | – | – |
| Hunt & Reffert (2024) | 113.581 | -17.187 | 0.608 | -3.271 | 1.009 | – |
| UCC | 113.645 | -17.168 | 0.607 | -3.251 | 0.983 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.8, m-M=11.0, logAge=7.7 |
| Hunt & Reffert (2023) | AV50=0.297, diffAV50=1.107, MOD50=10.917, logAge50=8.687 |
| Cavallo et al. (2024) | AV50=0.51, dMod50=10.91, logAge50=8.63, [Fe/H]50=-0.01 |
| Hunt & Reffert (2024) | MassJ=79.0223, MassTot=119.447 |
Search coordinates in Bayestar19
