CWNU 3857
Summary
CWNU 3857 is a sparse, very loose object of low C3 quality. It is located at a very 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) | 296.771 | 30.358 | 0.089 | -2.099 | -3.788 | -86.14 |
| UCC | 296.775 | 30.376 | 0.089 | -2.099 | -3.807 | -38.372 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.1, m-M=14.25, logA=9.1 |
Search coordinates in Bayestar19