CWNU 3470
Summary
CWNU 3470 is a poorly populated, loose object of intermediate C3 quality. It is located at a large distance from the Sun, 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) | 100.873 | -1.269 | 0.194 | -0.509 | 0.616 | 56.73 |
| UCC | 100.864 | -1.269 | 0.189 | -0.5 | 0.614 | 63.731 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.2, m-M=13.35, logA=7.4 |
Search coordinates in Bayestar19