CWNU 4453
Summary
CWNU 4453 is a sparse, moderately dense object of low C3 quality. It is located at a moderate 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) | 243.765 | -52.419 | 0.281 | -2.804 | -3.849 | -41.79 |
| UCC | 243.763 | -52.407 | 0.275 | -2.804 | -3.842 | -55.986 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.95, m-M=12.7, logA=6.0 |
Search coordinates in Bayestar19