CWNU 4812
Summary
CWNU 4812 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) | 301.172 | 38.895 | 0.12 | -2.143 | -3.408 | – |
| UCC | 301.16 | 38.891 | 0.117 | -2.119 | -3.416 | -100.262 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=0.75, m-M=16.05, logA=9.6 |
Search coordinates in Bayestar19