CWNU 4872
Summary
CWNU 4872 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well 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) | 272.807 | -25.877 | 0.1 | -2.747 | -5.599 | – |
| UCC | 272.803 | -25.875 | 0.094 | -2.753 | -5.597 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.9, m-M=14.35, logA=9.9 |
Search coordinates in Bayestar19