CWNU 3488
Summary
CWNU 3488 is a poorly populated, very loose object of high C3 quality. It is located at a large distance from the Sun, well 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) | 105.893 | -18.567 | 0.141 | -0.483 | 1.689 | 84.42 |
| UCC | 105.887 | -18.556 | 0.142 | -0.462 | 1.677 | 84.417 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.45, m-M=14.05, logA=7.5 |
Search coordinates in Bayestar19