CWNU 3762
Summary
CWNU 3762 is a sparse, very loose object of very low 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) | 331.245 | 57.295 | 0.171 | -2.679 | -2.067 | -62.91 |
| UCC | 331.256 | 57.294 | 0.158 | -2.695 | -2.053 | -62.913 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=3.7, m-M=14.55, logA=7.0 |
Search coordinates in Bayestar19