CWNU 200
Summary
CWNU 200 is a poorly populated, very dense object of high C3 quality. It is located at a relatively 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 a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 96.95 | 36.031 | 0.83 | -0.37 | -3.64 | -17.2 |
| He et al. (2022) | 96.949 | 36.046 | 0.833 | -0.37 | -3.614 | – |
| UCC | 96.937 | 36.036 | 0.825 | -0.371 | -3.616 | -15.111 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.3, m-M=10.3, logAge=8.8, Z=0.02 |
| He et al. (2022) | A0=0.75, logAge=7.55 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 3747 | 96.9 | 96.94 | 36.04 | 0.83 | -0.37 | -3.62 | -15.11 | 0.0 |