CWNU 444
Summary
CWNU 444 is a poorly populated, very loose object of high 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 a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 309.476 | 54.518 | 1.24 | -3.1 | -6.69 | -35.1 |
| UCC | 309.463 | 54.402 | 1.224 | -3.109 | -6.732 | -20.545 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.45, m-M=9.3, logAge=7.9, Z=0.018 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 199 | 87.5 | 309.43 | 54.51 | 1.22 | -3.1 | -6.73 | -20.54 | 0.08 |