CWNU 3879
Summary
CWNU 3879 is a sparse, loose object of very low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 104.645 | -1.312 | 0.214 | -0.124 | 0.401 | 71.94 |
| UCC | 104.645 | -1.317 | 0.184 | -0.122 | 0.411 | 96.959 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.45, m-M=12.85, logA=8.8 |
Search coordinates in Bayestar19