CWNU 3622
Summary
CWNU 3622 is a poorly populated, very loose object of high C3 quality. It is located at a large distance from the Sun, above 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) | 123.697 | -29.419 | 0.187 | -2.432 | 3.029 | – |
| UCC | 123.708 | -29.432 | 0.176 | -2.437 | 3.008 | 90.137 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.45, m-M=13.1, logA=8.9 |
Search coordinates in Bayestar19