CWNU 1850
Summary
CWNU 1850 is a sparse, very loose object of very low C3 quality. It is located at a relatively close 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) | 205.288 | -52.767 | 0.513 | -7.38 | -1.874 | -52.02 |
| UCC | 205.272 | -52.807 | 0.542 | -7.367 | -1.857 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.7, m-M=11.8, logAge=9.15 |
Search coordinates in Bayestar19