CWNU 1805
Summary
CWNU 1805 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, below 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) | 125.954 | -42.699 | 0.564 | -4.334 | 3.925 | – |
| UCC | 125.9 | -42.746 | 0.56 | -4.324 | 3.924 | 39.702 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.05, m-M=11.4, logAge=7.05 |
Search coordinates in Bayestar19