CWNU 4784
Summary
CWNU 4784 is a sparse, very loose object of low C3 quality. It is located at a large 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) | 287.981 | 3.69 | 0.114 | -2.996 | -5.726 | 62.92 |
| UCC | 288.007 | 3.718 | 0.126 | -2.985 | -5.708 | 33.544 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.3, m-M=14.95, logA=9.6 |
Search coordinates in Bayestar19