CWNU 3756
Summary
CWNU 3756 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.
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) | 106.186 | -16.112 | 0.079 | -0.477 | 1.047 | 83.94 |
| UCC | 106.178 | -16.116 | 0.066 | -0.488 | 1.038 | 83.935 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.7, m-M=14.3, logA=8.2 |
Search coordinates in Bayestar19