CWNU 4650
Summary
CWNU 4650 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, below 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) | 200.491 | -63.937 | 0.118 | -5.63 | -0.833 | – |
| UCC | 200.527 | -63.912 | 0.121 | -5.641 | -0.809 | 31.784 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.6, m-M=15.25, logA=10.1 |
Search coordinates in Bayestar19