CWNU 4574
Summary
CWNU 4574 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, 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) | 208.571 | -59.038 | 0.162 | -7.117 | -2.168 | – |
| UCC | 208.588 | -59.038 | 0.168 | -7.089 | -2.107 | 6.598 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.1, m-M=14.85, logA=9.8 |
Search coordinates in Bayestar19