CWNU 3518
Summary
CWNU 3518 is a sparse, very loose object of very low C3 quality. It is located at a moderate 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) | 96.24 | 27.969 | 0.225 | -0.118 | -1.535 | 35.69 |
| UCC | 96.271 | 27.936 | 0.221 | -0.119 | -1.535 | 17.485 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.0, m-M=13.0, logA=9.0 |
Search coordinates in Bayestar19