CWNU 1693
Summary
CWNU 1693 is a sparse, very loose object of very low C3 quality. It is located at a relatively close 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) | 66.595 | 46.702 | 0.614 | 1.129 | -1.963 | – |
| UCC | 66.459 | 46.769 | 0.564 | 1.152 | -1.956 | -7.681 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.85, m-M=11.1, logAge=7.15 |
Search coordinates in Bayestar19