CWNU 4370
Summary
CWNU 4370 is a sparse, very loose 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) | 271.55 | -25.959 | 0.226 | -0.118 | -0.929 | – |
| UCC | 271.541 | -25.932 | 0.243 | -0.113 | -0.93 | -17.956 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.85, m-M=12.75, logA=8.8 |
Search coordinates in Bayestar19