CWNU 4893
Summary
CWNU 4893 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above 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) | 266.242 | -13.63 | 0.141 | -2.032 | -4.799 | 48.95 |
| UCC | 266.221 | -13.626 | 0.165 | -2.024 | -4.767 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.6, m-M=15.9, logA=10.1 |
Search coordinates in Bayestar19