CWNU 4103
Summary
CWNU 4103 is a poorly populated, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above 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) | 162.998 | -58.461 | 0.217 | -5.602 | 2.485 | 7.53 |
| UCC | 163.004 | -58.46 | 0.21 | -5.601 | 2.498 | 6.606 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.3, m-M=12.9, logA=8.3 |
Search coordinates in Bayestar19