CWNU 414
Summary
CWNU 414 is a poorly populated, very loose object of intermediate C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 19.927 | 72.254 | 1.12 | -2.01 | -0.66 | 1.6 |
| UCC | 20.01 | 72.227 | 1.127 | -1.988 | -0.628 | -11.313 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | AG=0.35, m-M=9.3, logAge=8.9, Z=0.02 |
Search coordinates in Bayestar19