CWNU 1418
Summary
CWNU 1418 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 316.784 | 46.81 | 0.422 | -4.005 | -4.438 | – |
| UCC | 316.778 | 46.802 | 0.417 | -4.006 | -4.451 | 13.531 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.8, m-M=11.8, logAge=9.45 |
Search coordinates in Bayestar19