CWNU 4213
Summary
CWNU 4213 is a moderately populated, very loose object of low C3 quality. It is located at a very large distance from the Sun, well below 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. (2023) | 138.383 | -54.999 | 0.058 | -2.66 | 2.952 | – |
| UCC | 138.382 | -55.003 | 0.055 | -2.674 | 2.967 | 103.628 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.9, m-M=14.1, logA=9.7 |
Search coordinates in Bayestar19