CWNU 1609
Summary
CWNU 1609 is a poorly populated, very loose object of intermediate 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: 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) | 311.428 | 31.964 | 0.657 | -2.357 | -3.66 | -10.25 |
| UCC | 311.449 | 31.953 | 0.658 | -2.356 | -3.656 | -9.7 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.35, m-M=10.8, logAge=7.4 |
Search coordinates in Bayestar19