CWNU 4250
Summary
CWNU 4250 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) | 210.371 | -65.519 | 0.011 | -4.467 | -1.244 | 55.52 |
| UCC | 210.371 | -65.519 | 0.017 | -4.462 | -1.239 | 55.523 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.45, m-M=15.75, logA=9.5 |
Search coordinates in Bayestar19