CWNU 4446
Summary
CWNU 4446 is a poorly populated, very loose object of 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: 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) | 156.907 | -54.861 | 0.139 | -4.855 | 3.076 | – |
| UCC | 156.881 | -54.879 | 0.16 | -4.855 | 3.049 | 64.579 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.6, m-M=14.1, logA=9.4 |
Search coordinates in Bayestar19