CWNU 512
Summary
CWNU 512 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with at least one entry reported in the same catalogue.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 6.213 | 68.937 | 1.05 | -2.8 | -0.01 | – |
| Hunt & Reffert (2023) | 5.095 | 68.734 | 1.046 | -2.845 | -0.155 | -23.788 |
| Cavallo et al. (2024) | 4.603 | 68.921 | 1.044 | – | – | – |
| Hunt & Reffert (2024) | 5.095 | 68.734 | 1.046 | -2.845 | -0.155 | -23.788 |
| UCC | 5.086 | 68.902 | 1.05 | -2.847 | -0.142 | -21.482 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=2.2, m-M=10.9, logAge=6.5, Z=0.002 |
| Hunt & Reffert (2023) | AV50=2.929, diffAV50=1.845, MOD50=9.779, logAge50=7.97 |
| Cavallo et al. (2024) | AV50=3.03, dMod50=10.22, logAge50=7.55, [Fe/H]50=0.21 |
| Hunt & Reffert (2024) | MassJ=70.4268, MassTot=147.849 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 343 | 84.0 | 4.53 | 68.9 | 1.05 | -2.85 | -0.19 | -23.56 | 0.14 |
