CWNU 4473
Summary
CWNU 4473 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) | 308.735 | 51.935 | 0.086 | -2.598 | -2.982 | -74.4 |
| UCC | 308.752 | 51.95 | 0.1 | -2.57 | -2.949 | -88.077 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.4, m-M=13.95, logA=9.5 |
Search coordinates in Bayestar19