CWNU 3579
Summary
CWNU 3579 is a poorly populated, very loose object of intermediate 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) | 111.68 | -27.36 | 0.097 | -1.011 | 1.738 | 149.33 |
| UCC | 111.685 | -27.349 | 0.065 | -0.999 | 1.688 | 149.327 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.4, m-M=14.9, logA=8.8 |
Search coordinates in Bayestar19