CWNU 3850
Summary
CWNU 3850 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) | 323.818 | 57.285 | 0.12 | -2.632 | -2.333 | -68.42 |
| UCC | 323.782 | 57.281 | 0.109 | -2.647 | -2.333 | -92.354 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.65, m-M=13.7, logA=8.9 |
Search coordinates in Bayestar19