CWNU 3898
Summary
CWNU 3898 is a poorly populated, very loose object of intermediate C3 quality. It is located at a large 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. (2023) | 61.873 | 54.081 | 0.184 | -0.006 | 0.075 | – |
| UCC | 61.866 | 54.079 | 0.191 | -0.023 | 0.083 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.5, m-M=13.7, logA=7.4 |
Search coordinates in Bayestar19