CWNU 4218
Summary
CWNU 4218 is a poorly populated, very loose object of high C3 quality. It is located at a large distance from the Sun, 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) | 115.08 | -30.152 | 0.111 | -1.035 | 2.13 | – |
| UCC | 115.094 | -30.157 | 0.112 | -1.027 | 2.105 | 101.359 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.5, m-M=14.65, logA=8.8 |
Search coordinates in Bayestar19