CWNU 1701
Summary
CWNU 1701 is a sparse, loose object of very low C3 quality. It is located at a moderate 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) | 71.812 | 46.917 | 0.31 | 0.657 | -1.267 | -27.49 |
| UCC | 71.849 | 46.931 | 0.274 | 0.651 | -1.289 | -58.654 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=2.7, m-M=12.0, logAge=8.8 |
Search coordinates in Bayestar19